2021 
"Distribution of the total angular momentum in relativistic configurations" Poirier M & Pain JC, Journal of Physics B: Atomic, Molecular and Optical Physics.., jul, 2021. IOP Publishing, (2021). 
Abstract: This paper is devoted to the analysis of the distribution of the total angular momentum in a relativistic configuration. Using cumulants and generating function formalism this analysis can be reduced to the study of individual subshells with N equivalent electrons of momentum j. An expression as a nthderivative is provided for the generating function of the J distribution and efficient recurrence relations are established. It is shown that this distribution may be represented by a GramCharlierlike series which is derived from the corresponding series for the magnetic quantum number distribution. The numerical efficiency of this expansion is fair when the configuration consists of several subshells, while the accuracy is less good when only one subshell is involved. An analytical expression is given for the oddorder momenta while the evenorder ones are expressed as a series which provides an acceptable accuracy though being not convergent. Such expressions may be used to obtain approximate values for the number of transitions in a spinorbit split array: it is shown that the approximation is often efficient when few terms are kept, while some complex cases require to include a large number of terms. 
BibTeX:
@article{Poirier_2021, author = {Michel Poirier and JeanChristophe Pain}, title = {Distribution of the total angular momentum in relativistic configurations}, journal = {Journal of Physics B: Atomic, Molecular and Optical Physics}, publisher = {IOP Publishing}, year = {2021}, url = {https://doi.org/10.1088/13616455/ac17cb}, doi = {10.1088/13616455/ac17cb} } 
"Angular momentum distribution in a relativistic configuration: magnetic quantum number analysis" Poirier M & Pain JC, Journal of Physics B: Atomic, Molecular and Optical Physics., jul, 2021. Vol. 54(14), pp. 145002. IOP Publishing. (2021). 
Abstract: This paper is devoted to the analysis of the distribution of the total magnetic quantum number M in a relativistic subshell with N equivalent electrons of momentum j. This distribution is analyzed through its cumulants and through their generating function, for which an analytical expression is provided. This function also allows us to get the values of the cumulants at any order. Such values are useful to obtain the moments at various orders. Since the cumulants of the distinct subshells are additive this study directly applies to any relativistic configuration. Recursion relations on the generating function are given. It is shown that the generating function of the magnetic quantum number distribution may be expressed as an nth derivative of a polynomial. This leads to recurrence relations for this distribution which are very efficient even in the case of large j or N. The magnetic quantum number distribution is numerically studied using the GramCharlier and Edgeworth expansions. The inclusion of highorder terms may improve the accuracy of the GramCharlier representation for instance when a small and a large angular momenta coexist in the same configuration. However such series does not exhibit convergence when high orders are considered and the account for the first two terms often provides a fair approximation of the magnetic quantum number distribution. The Edgeworth series offers an interesting alternative though this expansion is also divergent and of asymptotic nature. 
BibTeX:
@article{Poirier2021, author = {Michel Poirier and JeanChristophe Pain}, title = {Angular momentum distribution in a relativistic configuration: magnetic quantum number analysis}, journal = {Journal of Physics B: Atomic, Molecular and Optical Physics}, publisher = {IOP Publishing}, year = {2021}, volume = {54}, number = {14}, pages = {145002}, url = {https://doi.org/10.1088/13616455/ac10f9}, doi = {10.1088/13616455/ac10f9} } 
2020 
"Analytical and numerical expressions for the number of atomic configurations contained in a supershell" Pain JC & Poirier M, Journal of Physics B: Atomic, Molecular and Optical Physics. Vol. 53, pp. 115002. IOP Publishing, (2020). 
Abstract: We present three explicit formulas for the number of electronic configurations in an atom, i.e. the number of ways to distribute Q electrons in N subshells of respective degeneracies g _{1}, g _{2}, ..., g _{N}. The new expressions are obtained using the generatingfunction formalism. The first one contains sums involving multinomial coefficients. The second one relies on the idea of gathering subshells having the same degeneracy. A third one also collects subshells with the same degeneracy and leads to the definition of a twovariable generating function, allowing the derivation of recursion relations. All these formulas can be expressed as summations of products of binomial coefficients. Concerning the distribution of population on N distinct subshells of a given degeneracy g, analytical expressions for the first moments of this distribution are given. The general case of subshells with any degeneracy is analysed through the computation of cumulants. A fairly simple expression for the cumulants at any order is provided, as well as the cumulant generating function. Using GramCharlier expansion, simple approximations of the analysed distribution in terms of a normal distribution multiplied by a sum of Hermite polynomials are given. These GramCharlier expansions are tested at various orders and for various examples of supershells. When few terms are kept they are shown to provide simple and efficient approximations of the distribution, even for moderate values of the number of subshells, though such expansions diverge when higher order terms are accounted for. The Edgeworth expansion has also been tested. Its accuracy is equivalent to the GramCharlier accuracy when few terms are kept, but it is much more rapidly divergent when the truncation order increases. While this analysis is illustrated by examples in atomic supershells it also applies to more general combinatorial problems such as fermion distributions. 
BibTeX:
@article{Pain2020, author = {JeanChristophe Pain and Michel Poirier}, title = {Analytical and numerical expressions for the number of atomic configurations contained in a supershell}, journal = {Journal of Physics B: Atomic, Molecular and Optical Physics}, publisher = {IOP Publishing}, year = {2020}, volume = {53}, pages = {115002}, url = {https://doi.org/10.1088/13616455/ab81ea}, doi = {10.1088/13616455/ab81ea} } 
2019 
"ExtremeUV absorption processes in a laserproduced midZ plasma: Measurements and theoretical interpretation" Poirier M, BastianiCeccotti S, Blenski T, Comet M, Esnault C, Gilleron F, Gilles D, Pain JC, Reverdin C et Thais F, High Energy Density Physics. Vol. 33, pp. 100706. (2019). 
Abstract: A good knowledge of absorption properties of plasmas at temperature of few tens of eV is essential in several domains such as astrophysics and inertial fusion science. For instance the description of stellar envelopes or the analysis of betaCephei pulsation requires an accurate determination of the Rosseland absorption coefficient, which strongly depends on the radiative properties of plasmas in the extremeUV (XUV) range. Contrary to measurements in Xray range, the literature on the absorption properties of plasmas of midZ elements in XUV domain is less abundant. Furthermore the theoretical interpretation of such spectra represents a theoretical challenge since this energy range involves transition arrays from n equal 3 to 3 with an approximately halfopen 3d subshell and possibly other open spectator subshells which contain a huge number of lines. The aim of this paper is to describe an experiment recently performed on the LULI 2000 laser facility mostly devoted to measurements of the absorption in the 60  180eV spectral region in a copper plasma at a temperature of 10 to 30 eV and a density of few mg/cm3. The experimental scheme is based on an indirect heating of multilayer thin foils by two gold cavities irradiated by two nanosecond doubledfrequency beams with an energy of several hundreds of J. This scheme allows one to obtain moderate temperature and densitygradients and ensures conditions close to local thermodynamic equilibrium. The selfemission of cavities in XUV range is tentatively eliminated by the use of a timedependent detection. A preliminary interpretation of these measurements is proposed. This analysis relies on three different codes: the hybrid code SCORCG, the Flexible Atomic Code in detailed or configurationaverage mode, and the HULLAC code in level or configuration mode. A partial agreement is obtained between theory and experiment, though the account for temperature gradients is probably necessary to accurately describe the present measurements. 
BibTeX:
@article{Poirier2019, author = {M. Poirier and S. BastianiCeccotti and T. Blenski and M. Comet and C. Esnault and F. Gilleron and D. Gilles and J.C. Pain and C. Reverdin and F. Thais}, title = {ExtremeUV absorption processes in a laserproduced midZ plasma: Measurements and theoretical interpretation}, journal = {High Energy Density Physics}, year = {2019}, volume = {33}, pages = {100706}, url = {http://www.sciencedirect.com/science/article/pii/S1574181819300473}, doi = {10.1016/j.hedp.2019.100706} } 
"Simpler freeenergy functional of the DebyeHückel model of fluids and the nonuniqueness of freeenergy functionals in the theory of fluids" Piron R et Blenski T, Physical Review E., May, 2019. Vol. 99, pp. 052134. American Physical Society,(2019). 
Abstract: In previous publications [Piron and Blenski, Phys. Rev. E 94, 062128 (2016); Blenski and Piron, High Energy Density Phys. 24, 28 (2017)], the authors have proposed DebyeHückelapproximate freeenergy functionals of the pair distribution functions for onecomponent fluids and twocomponent plasmas. These functionals yield the corresponding DebyeHückel integral equations when they are minimized with respect to the pair distribution functions, lead to correct thermodynamic relations, and fulfill the virial theorem. In the present paper, we update our results by providing simpler functionals that have the same properties. We relate these functionals to the approaches of Lado [Phys. Rev. A 8, 2548 (1973)] and of Olivares and McQuarrie [J. Chem. Phys. 65, 3604 (1976)]. We also discuss briefly the nonuniqueness issue that is raised by these results. 
BibTeX:
@article{PhysRevE.99.052134, author = {Piron, R. and Blenski, T.}, title = {Simpler freeenergy functional of the DebyeHückel model of fluids and the nonuniqueness of freeenergy functionals in the theory of fluids}, journal = {Phys. Rev. E}, publisher = {American Physical Society}, year = {2019}, volume = {99}, pages = {052134}, url = {https://link.aps.org/doi/10.1103/PhysRevE.99.052134}, doi = {10.1103/PhysRevE.99.052134} } 
"Simultaneous Xray and XUV absorption measurements in nickel laserproduced plasma close to LTE" Dozières M, Thais F, BastianiCeccotti S, Blenski T, Comet M, Condamine F, Fariaut J, Gilleron F, Gilles D, Pain J, Poirier M, Reverdin C, Rosmej F, Silvert V, Soullié G et Villette B, High Energy Density Physics. Vol. 31, pp. 83  91, (2019). 
Abstract: We present an experiment performed in 2016 at the LULI2000 laser facility in which Xray and XUV absorption structures of nickel hot plasmas were measured simultaneously. Such experiments may provide stringent tests of the accuracy of plasma atomicphysics codes used to the modeling of plasmas close to local thermodynamic equilibrium. The experimental setup relies on a symmetric heating of the sample foil by two gold hohlraums in order to reduce the spatial gradients. The plasma conditions are characterized by temperatures between 10 and 20 eV and densities of the order of 10^{3} g/cm3–10^{2} g/cm^{3}. For the Xray part, we investigate the 2p3d and 2p4d transitions, and for the XUV part, we recorded the Δn = 0 (n = 3) transitions, which present a high sensitivity to plasma temperature. These latter transitions are of particular interest because, in midZ plasmas, they dominate the Planck and Rosseland mean opacities. Measured spectra are compared to calculations performed using the hybrid opacity code SCORCG and the Flexible Atomic Code (FAC). The influence of a spectator electron on the calculated spectra is analyzed using the latter code. 
BibTeX:
@article{Dozieres2019, author = {M. Dozières and F. Thais and S. BastianiCeccotti and T. Blenski and M. Comet and F. Condamine and J. Fariaut and F. Gilleron and D. Gilles and JC. Pain and M. Poirier and C. Reverdin and F. Rosmej and V. Silvert and G. Soullié and B. Villette}, title = {Simultaneous Xray and XUV absorption measurements in nickel laserproduced plasma close to LTE}, journal = {High Energy Density Physics}, year = {2019}, volume = {31}, pages = {83  91}, url = {http://www.sciencedirect.com/science/article/pii/S1574181818300909}, doi = {10.1016/j.hedp.2019.03.007} } 
2018 
"Opacity calculations in X and XUV range using a detailed atomic code" Poirier M , Contributions to Plasma Physics. Vol. 58(10), pp. 10051014, (2018). 
Abstract: Calculations of accurate opacities in X and XUV range are of high interest for several domains such as astrophysics or inertial fusion science. Such quantities may be investigated through laserplasma interaction in the indirectdrive scheme. In this work absorption properties of such plasmas are analysed using the Flexible Atomic Code. Detailed and unresolvedtransitionarray modes are investigated, and some results obtained with the mixed mode recently developed are also proposed. For a carbon plasma the present approach agrees with the results obtained with the superconfiguration code SCO. Some results are provided about the Xray opacity of nickel, and a comparison with data from a recent campaign on LULI 2000 facility is done. This comparison demonstrates that the Unresolved Transition Array approach may be insufficient, e.g., to determinate the accurate position and shape of the 2p3d structure in nickel at about 25 eV. The case of nonelectricdipoletype transitions, such as magnetic dipole transitions is addressed. The electricdipole and magneticdipole transitions are studied here in the case of the 3 * n complex of five tungsten ions, with charge states similar to those found in the tokamak divertors. It is demonstrated that the unresolved transition array formulas provide a fairly accurate description of the most important absorption structures, but fail to reproduce correctly the behavior of the opacity in the wings of these main structures.. 
BibTeX:
@article{Poirier, author = {Poirier, M.}, title = {Opacity calculations in X and XUV range using a detailed atomic code}, journal = {Contributions to Plasma Physics}, year = {2018}, volume = {58}, number = {10}, pages = {10051014}, url = {https://onlinelibrary.wiley.com/doi/abs/10.1002/ctpp.201700070}, doi = {10.1002/ctpp.201700070} } 
"Average atom model calculations of dense plasma opacities: Review and potential applications to white dwarf stars"Piron R et Blenski T, Contributions to Plasma Physics. Vol. 58(1), pp. 3041, (2018). 
Abstract: Methods using average atom models in order to calculate dense plasma opacities and conductivities are reviewed. Dense plasmas at moderate temperatures, of interest in white dwarf modelling, are considered. Due to their relative simplicity of implementation, compared to more detailed models (detailed level accounting, detailed configuration accounting, etc.), average atom models are a privileged framework for the application of the most involved dense plasma statistical modelling. Moreover, the average atom models are well suited to the calculation of some thermodynamic properties, such as the equation of state. They can also be used in order to estimate broadband radiative properties of dense plasmas. After an introduction to the opacity issue in the modelling of white dwarfs, we make a short review of average atom models. We then address the methods of calculating the opacity starting from the average atom model, see some of their limitations, and briefly discuss some problems that remain open, such as the modelling of fluctuations, or the accounting for channel mixing and collective phenomena in the photoabsorption. 
BibTeX:
@article{doi:10.1002/ctpp.201700095, author = {Piron R. and Blenski T.}, title = {Average atom model calculations of dense plasma opacities: Review and potential applications to white dwarf stars}, journal = {Contributions to Plasma Physics}, year = {2018}, volume = {58}, number = {1}, pages = {3041}, url = {https://onlinelibrary.wiley.com/doi/abs/10.1002/ctpp.201700095}, doi = {10.1002/ctpp.201700095} } 
2017 
"Spectroscopic Study of Highly Ionised Plasmas : Detailed and Statistical Approaches" Na X, Thesis at: Université Paris XI  Paris Sud, (2017). 
Abstract: La description des propriétésspectrales des plasmas hautement ionisés –comme ceux rencontrés en fusion nucléaire,en astrophysique et en expérimentationlaserplasmas –peut nécessiter différentstypes d’interprétation, parmi lesquelsl’approche détaillée ou raieparraieimpliquant de la diagonalisation del’Hamiltonien du système et, l’approchestatistique basée sur la caractérisation desstructures spectrales à travers les momentsde distribution.Ce travail de thèse a pour objectif d'étudier etde mettre en œuvre les méthodes statistiquestraitant des cas où de nombreuses raies seregroupent en faisceaux de transition nonrésolus (UTA pour Unresolved TransitionArray).Pour cela, des études analytique et numériqueont été menées. D’une part, les momentsd’ordre élevé de la distribution d’énergies spinorbiteont été obtenus, en utilisant lestechniques de calcul de moyennes qui fontintervenir les résultats de la secondequantification et de l’algèbre de momentangulaire. D’autre part, après avoir implémentéun programme de posttraitement des donnéesatomiques produites par le code FAC (FlexibleAtomic Code), en mode détaillée comme enmode UTA, les spectres d’émission et... 
BibTeX:
@phdthesis{Na2017, author = {Na, Xieyu}, title = {Spectroscopic Study of Highly Ionised Plasmas : Detailed and Statistical Approaches}, school = {Université Paris XI  Paris Sud}, year = {2017}, note = {http://www.theses.fr/2017SACLS592}, url = {https://tel.archivesouvertes.fr/tel01696804} } 
"SuperConfigurationAccounting Equation of State for WDM and HED Plasma" Lee TG, Busquet M, Gilles D et Klapisch M, In American Phys. Soc. 62, 235, NP11.00050, (2017). 
Abstract: RadHydro numerical codes require Equation of State (EOS) and opacities. We describe a procedure to obtain an EOS compatible with our STA opacity model. We use our relativistic superconfiguration code  STA2.5 [1] to compute the average textless Ztextgreater and excitationionization internal energy U and chemical potential textunderscore . These and other data will serve as basic inputs into a Yukawa MonteCarlo [2] improved version of quotidian EOS [3], known as YMCQ. The screening in the Yukawa potential describing the ionion interaction is modified by the data from STA. This integrated procedure yields the excess internal energy due to the nonideal behavior of the EOS concordant with our opacity model and allows us to have an EOS model applicable from solid matter to very tenuous plasmas as found in laser fusion, astrophysics, or tokamaks. We shall present its application to Carbon, Aluminum and Iron. [1] M. Busquet, M. Klapisch, Bull. American Phys. Soc. 55, 225 (2010) [2] D. Gilles, F. Lambert, J. Clérouin, G. Salin, HEDP 3, 95 (2007); J. M. Caillol, D. Gilles, J. Stat. Phys. 100, 933 (2000) [3] D. M. More, K. H. Warren, D. A. Young, and G. B. Zimmerman, Phys. Fluids 31, 3059 (1998) 
BibTeX:
@conference{Lee2017, author = {T.G. Lee, M. Busquet, D. Gilles, M. Klapisch}, title = {SuperConfigurationAccounting Equation of State for WDM and HED Plasma}, booktitle = {American Phys. Soc. 62, 235, NP11.00050}, year = {2017}, url = {http://meetings.aps.org/Meeting/DPP17/Event/309662} } 
"Freeenergy functional of the DebyeHückel model of twocomponent plasmas" Blenski T et Piron R, High Energy Density Physics. Vol. 24(Supplement C), pp. 28  32, (2017) 
Abstract: Abstract We present a generalization of the DebyeHückel freeenergydensity functional of simple fluids to the case of twocomponent systems with arbitrary interaction potentials. It allows one to obtain the twocomponent DebyeHückel integral equations through its minimization with respect to the pair correlation functions, leads to the correct form of the internal energy density, and fulfills the virial theorem. It is based on our previous idea, proposed for the onecomponent DebyeHückel approach, which was published recently in Ref. [1]. We use the DebyeKirkwood charging method in the same way as in Ref. [1], in order to build an expression of the freeenergy density functional. Main properties of the twocomponent DebyeHückel free energy are presented and discussed, including the virial theorem in the case of longrange interaction potentials. 
BibTeX:
@article{Blenski2017, author = {T. Blenski and R. Piron}, title = {Freeenergy functional of the DebyeHückel model of twocomponent plasmas}, journal = {High Energy Density Physics}, year = {2017}, volume = {24}, number = {Supplement C}, pages = {28  32}, url = {http://www.sciencedirect.com/science/article/pii/S1574181817300423}, doi = {10.1016/j.hedp.2017.05.005} } 
"Analysis of magneticdipole transitions in tungsten plasmas using detailed and configurationaverage descriptions" Na, X. & Poirier, M., High Energy Density Physics ., June, 2017. Vol. 23, p 200  206, (2017). 
Abstract: This paper is devoted to the analysis of transition arrays of magneticdipole (M_{1}) type in highly charged ions. Such transitions play a significant role in highly ionized plasmas, for instance in the tungsten plasma present in tokamak devices. Using formulas recently published and their implementation in the Flexible Atomic Code for M_{1}transition array shifts and widths, absorption and emission spectra arising from transitions inside the 3*n complex of highlycharged tungsten ions are analyzed. A comparison of magneticdipole transitions with electricdipole (E_{1}) transitions shows that, while the latter are better described by transition array formulas, M_{1} absorption and emission structures reveal some insufficiency of these formulas. It is demonstrated that the detailed spectra account for significantly richer structures than those predicted by the transition array formalism. This is due to the fact that M_{1} transitions may occur between levels inside the same relativistic configuration, while such inner configuration transitions are not accounted for by the currently available averaging expression. In addition, because of configuration interaction, transition processes involving more than one electron jump, such as 3p_{1/2}3d_{5/2} > 3p_{3/2}3d_{3/2}, are possible but not accounted for in the transition array formulas. These missing transitions are collected in pseudoarrays using a postprocessing method described in this paper. The relative influence of inner and interconfiguration transitions is carefully analyzed in cases of tungsten ions with net charge around 50. The need for an additional theoretical development is emphasized. 
BibTeX:
@ARTICLE{Na2017200, author = {Xieyu Na and Michel Poirier}, title = {Analysis of magneticdipole transitions in tungsten plasmas using detailed and configurationaverage descriptions }, journal = {High Energy Density Physics }, year = {2017}, volume = {23}, pages = {200  206}, abstract = {Abstract This paper is devoted to the analysis of transition arrays of magneticdipole (M_{1}) type in highly charged ions. Such transitions play a significant role in highly ionized plasmas, for instance in the tungsten plasma present in tokamak devices. Using formulas recently published and their implementation in the Flexible Atomic Code for M_{1}transition array shifts and widths, absorption and emission spectra arising from transitions inside the 3*n complex of highlycharged tungsten ions are analyzed. A comparison of magneticdipole transitions with electricdipole (E_{1}) transitions shows that, while the latter are better described by transition array formulas, M_{1} absorption and emission structures reveal some insufficiency of these formulas. It is demonstrated that the detailed spectra account for significantly richer structures than those predicted by the transition array formalism. This is due to the fact that M_{1} transitions may occur between levels inside the same relativistic configuration, while such inner configuration transitions are not accounted for by the currently available averaging expression. In addition, because of configuration interaction, transition processes involving more than one electron jump, such as 3p_{1/2}3d_{5/2} > 3p_{3/2}3d_{3/2}, are possible but not accounted for in the transition array formulas. These missing transitions are collected in pseudoarrays using a postprocessing method described in this paper. The relative influence of inner and interconfiguration transitions is carefully analyzed in cases of tungsten ions with net charge around 50. The need for an additional theoretical development is emphasized.}, doi = {10.1016/j.hedp.2017.05.004}, issn = {15741818}, keywords = {Magneticdipole transitions}, owner = {jubera}, timestamp = {2017.06.07}, url = {http://www.sciencedirect.com/science/article/pii/S1574181817300435} } 
"The hybrid detailed / statistical opacity code SCORCG: New developments and applications" Pain JC, Gilleron F, Porcherot Q et Blenski T, AIP Conference Proceedings., March, 2017. Vol. 1811(1), pp. 190010. American Institute of Physics, (2017). 
Abstract: We present the hybrid opacity code SCORCG which combines statistical approaches with finestructure calculations. Radial integrals needed for the computation of detailed transition arrays are calculated by the code SCO (Superconfiguration Code for Opacity), which calculates atomic structure at finite temperature and density, taking into account plasma effects on the wavefunctions. Levels and spectral lines are then computed by an adapted RCG routine of R. D. Cowan. SCORCG now includes the Partially Resolved Transition Array model, which allows one to replace a complex transition array by a smallscale detailed calculation preserving energy and variance of the genuine transition array and yielding improved highorder moments. An approximate method for studying the impact of strong magnetic field on opacity and emissivity was also recently implemented. 
BibTeX:
@article{Pain2017, author = {Pain, J.C. and Gilleron, F. and Porcherot, Q. and Blenski, T.}, title = {The hybrid detailed / statistical opacity code SCORCG: New developments and applications}, journal = {AIP Conference Proceedings}, publisher = {American Institute of Physics}, year = {2017}, volume = {1811}, number = {1}, pages = {190010}, url = {https://aip.scitation.org/doi/abs/10.1063/1.4975753}, doi = {10.1063/1.4975753} } 
"Kshell spectroscopy in hot plasmas: Stark effect, Breit interaction and QED corrections" Pain JC, Gilleron F, Comet M et Gilles D, AIP Conference Proceedings., March, 2017. Vol. 1811(1), pp. 040004. American Institute of Physics, (2017). 
Abstract: he broadening of lines by Stark effect is widely used for inferring electron density and temperature in plasmas. Starkeffect calculations often rely on atomic data (transition rates, energy levels,...) not always exhaustive and/or valid only for isolated atoms. In this work, we first present a recent development in the detailed opacity code SCORCG for Kshell spectroscopy. The approach is adapted from the work of Gilles and Peyrusse. Neglecting nondiagonal terms in dipolar and collision operators, the line profile is expressed as a sum of Voigt functions associated to the Stark components. The formalism relies on the use of parabolic coordinates and the relativistic fine structure of Lyman lines is included by diagonalizing the Hamiltonian matrix associated to quantum states having the same principal quantum number n. The SCORCG code enables one to investigate plasma environment effects, the impact of the microfield distribution, the decoupling between electron and ion temperatures and the role of satellite lines (such as Lilike 1snℓn′ℓ′ 1s^{2}nl, Belike, etc.). Atomic structure calculations have reached levels of accuracy which require evaluation of Breit interaction and manyelectron quantum electrodynamics (QED) contributions. Although much work was done for QED effects (selfenergy and vacuum polarization) in hydrogenic atoms, the case of an arbitrary number of electrons is more complicated. Since exact analytic solutions do not exist, a number of heuristic methods have been used to approximate the screening of additional electrons in the selfenergy part. We compare different ways of including such effects in atomicstructure codes (SlaterCondon, MultiConfiguration DiracFock, etc.). 
BibTeX:
@article{Pain2017a, author = {Pain, J.C. and Gilleron, F. and Comet, M. and Gilles, D.}, title = {Kshell spectroscopy in hot plasmas: Stark effect, Breit interaction and QED corrections}, journal = {AIP Conference Proceedings}, publisher = {American Institute of Physics}, year = {2017}, volume = {1811}, number = {1}, pages = {040004}, url = {https://aip.scitation.org/doi/abs/10.1063/1.4975720}, doi = {10.1063/1.4975720} } 
2016 
"Suprathermal electrons in kJlaser produced plasmas: M shell resolved highresolution xray spectroscopic study of transient matter evolution" Condamine FP, Šmíd M, Renner O, Dozières M, Thais F, Angelo P, Bobin JL et Rosmej FB, Journal of Physics: Conference Series. Vol. 717(1), pp. 012060, (2016). 
Abstract: Hot electrons are of key importance to understand many physical processes in plasma physics. They impact strongly on atomic physics as almost all radiative properties are seriously modified. Xray spectroscopy is of particular interest due to reduced photoabsorption in dense matter. We report on a study of the copper Ka Xray emission conducted at the ns, kJ laser facility PALS, Prague, Czech Republic. Thin copper foils have been irradiated with 1? pulses. Two spherically bent quartz Bragg crystal spectrometers with high spectral and spatial resolution have been set up simultaneously to achieve a high level of confidence in the spectral distribution. In particular, an emission on the red wing of the Ka 2 transition (λ = 1.5444 Å) could be identified with complex atomic structure calculations. We discuss possible implications for the analysis of nonequilibrium phenomena and present first atomic physics simulations. 
BibTeX:
@article{Condamine2016, author = {F P Condamine and M Šmíd and O Renner and M Dozières and F Thais and P Angelo and JL Bobin and F B Rosmej}, title = {Suprathermal electrons in kJlaser produced plasmas: M shell resolved highresolution xray spectroscopic study of transient matter evolution}, journal = {Journal of Physics: Conference Series}, year = {2016}, volume = {717}, number = {1}, pages = {012060}, url = {http://stacks.iop.org/17426596/717/i=1/a=012060}, doi = {10.1088/17426596/717/1/012060} } 
"Configuration interaction effect on open M shell Fe and Ni LTE spectral opacities, Rosseland and Planck means" Gilles D, Busquet M, Gilleron F, Klapisch M et Pain JC, Journal of Physics: Conference Series. Vol. 717(1), pp. 012017, (2016). 
Abstract: We have recently shown that iron and nickel open Mshell opacity spectra, up to Δn = 2 are very sensitive to Configuration Interaction (CI) treatments at temperature around 15 eV and for various densities. To do so we had compared extensive CI calculations obtained with two opacity codes HULLACv9 and SCORCG. In this work we extend these comparisons to a first evaluation of CI effects on Rosseland and Planck means. 
BibTeX:
@article{Gilles2016a, author = {D Gilles and M Busquet and F Gilleron and M Klapisch and JC Pain}, title = {Configuration interaction effect on open M shell Fe and Ni LTE spectral opacities, Rosseland and Planck means}, journal = {Journal of Physics: Conference Series}, year = {2016}, volume = {717}, number = {1}, pages = {012017}, url = {http://stacks.iop.org/17426596/717/i=1/a=012017}, doi = {10.1088/17426596/717/1/012017} } 
"Etude expérimentale du transport de l'énergie radiative dans les plasmas denses par spectroscopie d'absorption et d'émission" Dozières M , Thesis at: Université Paris XI  Paris Sud, (2016). 
Abstract: Ce travail de thèse est une étude expérimentale, basée sur la spectroscopie d’émission et d’absorption de plasmas chauds et denses créés par une impulsion laser nanoseconde. La physique atomique au sein de ce type de plasmas représente un sujet complexe et de grand intérêt, notamment dans les domaines de l’astrophysique ou de la fusion par confinement inertiel. Du point de vue de la physique atomique, cela revient à déterminer des paramètres tels que l’ionisation moyenne ou l’opacité en fonction de la température électronique et de la densité de matière du milieu. Les codes de physique atomique ont alors besoin de données expérimentales pour se développer et être validés afin qu’ils soient prédictifs sur une large gamme de plasmas. Dans ce travail nous nous concentrons sur des plasmas dont la température électronique varie de 10 eV à plus d’une centaine d’électronvolts pour des densités de matière allant de 10⁻⁵ à 10⁻² g/cm³. Dans ce manuscrit on distingue deux types de données spectroscopiques qui sont toutes les deux utiles et nécessaires au développement des codes de physique atomique car elles sont caractéristiques de l’état du plasma étudié : 1) des spectres d’absorption obtenus avec des plasmas proche de l’équilibre thermodynamique local de Cu, de Ni et d’Al ; 2) des spectres d’émission obtenus avec des plasmas hors équilibre thermodynamique local de C, d’Al et de Cu. Ce travail met en lumière différentes techniques expérimentales ainsi que diverses comparaisons avec des codes de physique atomique et d’hydrodynamique. 
BibTeX:
@phdthesis{Dozieres2016, author = {Dozières, M.}, title = {Étude expérimentale du transport de l’énergie radiative dans les plasmas denses par spectroscopie d'absorption et d'émission}, school = {Université Paris XI  Paris Sud}, year = {2016}, note = {http://www.theses.fr/2016SACLS454}, url = {https://tel.archivesouvertes.fr/tel01527622} } 
"Freeenergy functional of the DebyeHückel model of simple fluids" Piron R et Blenski T, Physical Review E., December, 2016. Vol. 94(6), pp. 062128. American Physical Society, (2016). 
Abstract: The DebyeHÃ¼ckel approximation to the free energy of a simple fluid is written as a functional of the pair correlation function. This functional can be seen as the DebyeHÃ¼ckel equivalent to the functional derived in the hypernetted chain framework by Morita and Hiroike, as well as by Lado. It allows one to obtain the DebyeHÃ¼ckel integral equation through a minimization with respect to the pair correlation function, leads to the correct form of the internal energy, and fulfills the virial theorem. 
BibTeX:
@article{Piron2016, author = {Piron, R. and Blenski, T.}, title = {Freeenergy functional of the DebyeHückel model of simple fluids}, journal = {Phys. Rev. E}, publisher = {American Physical Society}, year = {2016}, volume = {94}, number = {6}, pages = {062128}, url = {http://link.aps.org/doi/10.1103/PhysRevE.94.062128}, doi = {10.1103/PhysRevE.94.062128} } 
"Highorder moments of spinorbit energy in a multielectron configuration" Na X et Poirier M, Physical Review E., Jul, 2016. Vol. 94, pp. 013206. American Physical Society, (2016). 
Abstract: In order to analyze the energylevel distribution in complex ions such as those found in warm dense plasmas, this paper provides values for highorder moments of the spinorbit energy in a multielectron configuration. Using secondquantization results and standard angular algebra or fully analytical expressions, explicit values are given for moments up to 10th order for the spinorbit energy. Two analytical methods are proposed, using the uncoupled or coupled orbital and spin angular momenta. The case of multiple open subshells is considered with the help of cumulants. The proposed expressions for spinorbit energy moments are compared to numerical computations from Cowan's code and agree with them. The convergence of the GramCharlier expansion involving these spinorbit moments is analyzed. While a spectrum with infinitely thin components cannot be adequately represented by such an expansion, a suitable convolution procedure ensures the convergence of the GramCharlier series provided highorder terms are accounted for. A corrected analytical formula for the thirdorder moment involving both spinorbit and electronelectron interactions turns out to be in fair agreement with Cowan's numerical computations. 
BibTeX:
@article{PhysRevE.94.013206, author = {Na, Xieyu and Poirier, M.}, title = {Highorder moments of spinorbit energy in a multielectron configuration}, journal = {Phys. Rev. E}, publisher = {American Physical Society}, year = {2016}, volume = {94}, pages = {013206}, url = {http://link.aps.org/doi/10.1103/PhysRevE.94.013206}, doi = {10.1103/PhysRevE.94.013206} } 
"Dynamic linear response of atoms in plasmas and photoabsorption crosssection in the dipole approximation " Caizergues C, Blenski T et Piron R, High Energy Density Physics. Vol. 18, pp. 7  13, (2016), 
Abstract: Abstract We report results on the selfconsistent linear response theory of quantum averageatoms in plasmas. The approach is based on the two first orders of the cluster expansion of the plasma susceptibility. A change of variable is applied, which allows us to handle the diverging freefree transitions contribution in the selfconsistent induced electron density and potential. The method is first tested on the case of rare gas isolated neutral atoms. A test of the Ehrenfesttype sum rule is then performed in a case of an actual averageatom in a plasma. At frequencies much higher than the plasma frequency, the sum rule seems to be fulfilled within the accuracy of the numerical methods. Close to the plasma frequency, the method seems not to account for the coldplasma dielectric function renormalization in the sum rule, which was correctly reproduced in the case of the Thomasâ€“Fermiâ€“Bloch selfconsistent linear response. This suggests the need for a better accounting for the outgoing waves in the asymptotic boundary conditions. 
BibTeX:
@article{Caizergues20167, author = {C. Caizergues and T. Blenski and R. Piron}, title = {Dynamic linear response of atoms in plasmas and photoabsorption crosssection in the dipole approximation }, journal = {High Energy Density Physics }, year = {2016}, volume = {18}, pages = {7  13}, url = {http://www.sciencedirect.com/science/article/pii/S1574181815001032}, doi = {10.1016/j.hedp.2015.11.001} } 
2015 
"Xray opacity measurements in midZ dense plasmas with a new target design of indirect heating" Dozières M, Thais F, BastianiCeccotti S, Blenski T, Fariaut J, Fölsner W, Gilleron F, Khaghani D, Pain JC, Reverdin C, Rosmej F, Silvert V, Soullié G et Villette B, High Energy Density Physics., December, 2015. Vol. 17, Part B, pp. 231239. (2015). 
Abstract: Xray transmission spectra of copper, nickel and aluminum laser produced plasmas were measured at the LULI2000 laser facility with an improved target design of indirect heating. Measurements were performed in plasmas close to local thermodynamic equilibrium at temperatures around 25 eV and densities between 10−3 g/cm3 and 10−2 g/cm3. This improved design provides several advantages, which are discussed in this paper. The sample is a thin foil of midZ material inserted between two gold cavities heated by two 300J, 2ω, nanosecond laser beams. A third laser beam irradiates a gold foil to create a spectrally continuous Xray source (backlight) used to probe the sample. We investigate 2p–3d absorption structures in Ni and Cu plasmas as well as 1s–2p transitions in an additional Al plasma layer to infer the insitu plasma temperature. Geometric and hydrodynamic calculations indicate that the improved geometry reduces spatial gradients during the transmission measurements. Experimental absorption spectra are in good agreement with calculations from the hybrid atomic physics code SCORCG. 
BibTeX:
@article{Dozieres2015, author = {Dozières, M. and Thais, F. and BastianiCeccotti, S. and Blenski, T. and Fariaut, J. and Fölsner, W. and Gilleron, F. and Khaghani, D. and Pain, J.C. and Reverdin, C. and Rosmej, F. and Silvert, V. and Soullié, G. and Villette, B.}, title = {Xray opacity measurements in midZ dense plasmas with a new target design of indirect heating}, journal = {High Energy Density Physics}, year = {2015}, volume = {17, Part B}, pages = {231239}, url = {http://www.sciencedirect.com/science/article/pii/S157418181500066X} } 
"Precise Opacities for Astrophysics (Fe and Ni) and ICF modeling" Klapisch M, Gilles D et Busquet M, In 57th Annual Meeting of the APS Division of Plasma Physics, MondayFriday, November 1620, 2015; Savannah, Georgia, (Volume 60, Number 19), (2015). 
Abstract: Precise Opacities for Astrophysics (Fe and Ni) and ICF modeling MARCEL KLAPISCH, BRA, Beltsville, MD 21042, DOMINIQUE GILLES, CEA/IRFU/Sap, F91191, France, MICHEL BUSQUET, RSI, Lanham, MD 20706  Opacities of FeIII  FeXV at Te=1520 eV and densities 1.e161.e23 cm3 have been computed with an improved version of the HULLAC code [1, 2]. More than 109 transitions have been computed, with di?erent ways to account for con?guration interactions (CI). Spectra with CI limited to each nonrelativistic con?guration (CIinNRC) are compared to more extended full Relativistic CI (RCI). The e?ect of increasing the size of the CI basis is investigated. These comparisons enable optimizing the method for each temperature/density regime. With powerful computers, HULLAC generated opacity databases could then be envisioned, bypassing the need for statistical approximations. [1] D. Gilles, M. Busquet, M. Klapisch, F. Gilleron, J.C. Pain, Open Mshell Fe and Ni LTE opacity calculations with the code HULLACv9, High Ener. Dens. Phys., 16 (2015) 111. [2] M. Klapisch, M. Busquet, A. BarShalom, A New And Improved Version Of HULLAC, AIP Conference Proceedings, 926 (2007) 206215. 
BibTeX:
@conference{APS2015, author = {Marcel Klapisch and Dominique Gilles and Michel Busquet}, title = {Precise Opacities for Astrophysics (Fe and Ni) and ICF modeling}, booktitle = {57th Annual Meeting of the APS Division of Plasma Physics }, year = {2015}, number = {Volume 60, Number 19}, url = {http://meetings.aps.org/Meeting/DPP15/Session/UP12.16} } 
"Open Mshell Fe and Ni LTE opacity calculations with the code HULLACv9" Gilles D, Busquet M, Klapisch M, Gilleron F et Pain JC (2015), , High Energy Density Physics., September, 2015. Vol. 16, pp. 111. 
Abstract:It has been shown that a careful evaluation of the Δn = 0 Mshell in Fe and Ni is necessary to obtain consistent stellar model predictions. At astrophysical conditions of Te = 15.3 eV, ne = 1013 1022cm−3, the Δn = 0 Mshell and absorption transitions among M to N and M to O shells arising from the ions Fe III through Fe XV, have been computed in the using detailed level accounting (DLA) with configuration interaction (CI), assuming LTE. The importance of extensive CI computations is shown by systematically increasing the size of the CI basis until convergence. Iron opacity results, including Mshell and M to upper shells transitions up to Δn = 2, are presented and the influence of the number of atomic levels is discussed. These very large computations –e.g. ∼7.3 × 105 levels or ∼5700 relativistic configurations in Fe VII– were performed using the flexibility and the efficiency of an updated version of the HULLACv9.5 code. Results for Ni are also reported. HULLACv9.5 results are compared with those of other codes and databases, STA, SCORCG and OPCD3.3. 
BibTeX:
@article{Gilles2015, author = {Gilles, D. and Busquet, M. and Klapisch, M. and Gilleron, F. and Pain, J.C.}, title = {Open Mshell Fe and Ni LTE opacity calculations with the code HULLACv9}, journal = {High Energy Density Physics}, year = {2015}, volume = {16}, pages = {111}, url = {http://www.sciencedirect.com/science/article/pii/S1574181815000415}, doi = {10.1016/j.hedp.2015.04.008} } 
"Influence of the plasma environment on atomic structure using an ionsphere model" Belkhiri M, Fontes CJ et Poirier M , Phys. Rev. A., Sep, 2015. Vol. 92, pp. 032501. American Physical Society, (2015). 
Abstract: Plasma environment effects on atomic structure are analyzed using various atomic structure codes. To monitor the effect of high freeelectron density or low temperatures, FermiDirac and MaxwellBoltzmann statistics are compared. After a discussion of the implementation of the FermiDirac approach within the ionsphere model, several applications are considered. In order to check the consistency of the modifications brought here to extant codes, calculations have been performed using the Los Alamos Cowan Atomic Structure (cats) code in its HartreeFock or HartreeFockSlater form and the parametric potential Flexible Atomic Code (fac). The groundstate energy shifts due to the plasma effects for the six most ionized aluminum ions have been calculated using the fac and cats codes and fairly agree. For the intercombination resonance line in Fe22+, the plasma effect within the uniform electron gas model results in a positive shift that agrees with the multiconfiguration DiracFock value of B. Saha and S. Fritzsche [J. Phys. B 40, 259 (2007)]. Last, the present model is compared to experimental data in titanium measured on the terawatt Astra facility and provides values for electron temperature and density in agreement with the maria code. 
BibTeX:
@article{Belkhiri2015, author = {Belkhiri, Madeny and Fontes, Christopher J. and Poirier, Michel}, title = {Influence of the plasma environment on atomic structure using an ionsphere model}, journal = {Phys. Rev. A}, publisher = {American Physical Society}, year = {2015}, volume = {92}, pages = {032501}, url = {http://link.aps.org/doi/10.1103/PhysRevA.92.032501}, doi = {10.1103/PhysRevA.92.032501} } 
"Detailed computation of hotplasma atomic spectra" Pain JC, Gilleron F et Blenski T, Laser and Particle Beams. Vol. 33, pp. 201210, (2015). 
Abstract: We present recent evolutions of the detailed opacity code SCORCG which combines statistical modelings of levels and lines with finestructure calculations. The code now includes the Partially Resolved Transition Array model, which allows one to replace a complex transition array by a smallscale detailed calculation preserving energy and variance of the genuine transition array and yielding improved higherorder moments. An approximate method for studying the impact of strong magnetic field on opacity and emissivity was also recently implemented. The Zeeman line profile is modeled by fourthorder GramCharlier expansion series, which is a Gaussian multiplied by a linear combination of Hermite polynomials. Electron collisional line broadening is often modeled by a Lorentzian function and one has to calculate the convolution of a Lorentzian with GramCharlier distribution for a huge number of spectral lines. Since the numerical cost of the direct convolution would be prohibitive, we propose, to obtain the resulting profile, a fast and precise algorithm, relying on a representation of the Gaussian by cubic splines. 
BibTeX:
@article{Pain2015, author = {JeanChristophe Pain and Franck Gilleron and Thomas Blenski}, title = {Detailed computation of hotplasma atomic spectra}, journal = {Laser and Particle Beams}, year = {2015}, volume = {33}, pages = {201210}, url = {http://journals.cambridge.org/article_S0263034615000257}, doi = {10.1017/S0263034615000257} } 
"Réponse linéaire dynamique et autocohérente des atomes dans les plasmas quantiques : photoabsorption et effets collectifs dans les plasmas denses". Caizergues C, Thesis at: Université Paris XI  Paris Sud., (2015). 
Abstract: Dans la modélisation de la matière dense, et partiellement ionisée, une question importante concerne le traitement des électrons libres. Visàvis des électrons liés, la nature délocalisée et non discrète de ces électrons est responsable d'une différence de traitement, qui est souvent effectuée dans les modélisations des propriétés radiatives des plasmas. Cependant, afin d'éviter les incohérences dans le calcul des spectres d'absorption, tous les électrons devraient, en principe, être décrits dans un même formalisme. Nous utilisons deux modèles variationnels d'atomemoyen : un modèle semiclassique, et un modèle quantique, qui permettent cette égalité de traitement pour tous les électrons. Nous calculons la sectionefficace de photoextinction, en appliquant le cadre de la théorie de la réponse linéaire dynamique à chacun de ces modèles d'atome dans un plasma. Pour cette étude, nous développons et utilisons une approche autocohérente, de type randomphaseapproximation (RPA), qui, en allant audelà de la réponse des électrons indépendants, permet d'évaluer les effets collectifs, par l'introduction de la polarisation dynamique. Cette approche s'inscrit dans le formalisme de la théorie de la fonctionnelle de la densité dépendant du temps (TDDFT), appliquée au cas d'un système atomique immergé dans un plasma. Pour les deux modèles, semiclassique et quantique, nous dérivons, et vérifions dans nos calculs, une nouvelle règle de somme, qui permet d'évaluer le dipôle atomique à partir d'un volume fini dans le plasma. Cette règle de somme s'avère être un outil de premier ordre pour le calcul des propriétés radiatives des atomes dans les plasmas denses. 
BibTeX:
@phdthesis{Caizergues2015, author = {Caizergues, C.}, title = {Réponse linéaire dynamique et autocohérente des atomes dans les plasmas quantiques : photoabsorption et effets collectifs dans les plasmas denses}, school = {Université Paris XI  Paris Sud}, year = {2015}, note = {http://www.theses.fr/2015PA112042}, url = {https://tel.archivesouvertes.fr/tel011540568} } 
"A study of density effects in plasmas using analytical approximations for the selfconsistent potential" Poirier M, High Energy Density Physics. Vol. 15, pp. 12  21, (2015). 
Abstract: Abstract Density effects in ionized matter require particular attention since they modify energies, wavefunctions and transition rates with respect to the isolatedion situation. The approach chosen in this paper is based on the ionsphere model involving a ThomasFermilike description for free electrons, the bound electrons being described by a full quantum mechanical formalism. This permits to deal with plasmas out of thermal local equilibrium, assuming only a Maxwell distribution for free electrons. For Hlike ions, such a theory provides simple and rather accurate analytical approximations for the potential created by free electrons. Emphasis is put on the plasma potential rather than on the electron density, since the energies and wavefunctions depend directly on this potential. Beyond the uniform electron gas model, temperature effects may be analyzed. In the case of Hlike ions, this formalism provides analytical perturbative expressions for the energies, wavefunctions and transition rates. Explicit expressions are given in the case of maximum orbital quantum number, and compare satisfactorily with results from a direct integration of the radial Schrödinger equation. Some formulas for lower orbital quantum numbers are also proposed. 
BibTeX:
@article{Poirier2015, author = {M. Poirier}, title = {A study of density effects in plasmas using analytical approximations for the selfconsistent potential}, journal = {High Energy Density Physics}, year = {2015}, volume = {15}, pages = {12  21}, url = {http://www.sciencedirect.com/science/article/pii/S1574181815000245}, doi = {10.1016/j.hedp.2015.03.008} } 
2014 
"Analysis of density effects in plasmas and their influence on electronimpact cross sections" Belkhiri M and Poirier M, Phys. Rev. A., Dec, 2014. Vol. 90, pp. 062712. American Physical Society, (2014). 
Abstract: Density effects in plasmas are analyzed using a ThomasFermi approach for free electrons. First, scaling properties are determined for the freeelectron potential and density. For hydrogenlike ions, the first two terms of an analytical expansion of this potential as a function of the plasma coupling parameter are obtained. In such ions, from these properties and numerical calculations, a simple analytical fit is proposed for the plasma potential, which holds for any electron density, temperature, and atomic number, at least assuming that MaxwellBoltzmann statistics is applicable. This allows one to analyze perturbatively the influence of the plasma potential on energies, wave functions, transition rates, and electronimpact collision rates for singleelectron ions. Second, plasmas with an arbitrary charge state are considered, using a modified version of the Flexible Atomic Code (FAC) package with a plasma potential based on a ThomasFermi approach. Various methods for the collision crosssection calculations are reviewed. The influence of plasma density on these cross sections is analyzed in detail. Moreover, it is demonstrated that, in a given transition, the radiative and collisionalexcitation rates are differently affected by the plasma density. Some analytical expressions are proposed for hydrogenlike ions in the limit where the Born or Lotz approximation applies and are compared to the numerical results from the FAC. 
BibTeX:
@article{PhysRevA.90.062712, author = {Belkhiri, M. and Poirier, M.}, title = {Analysis of density effects in plasmas and their influence on electronimpact cross sections}, journal = {Phys. Rev. A}, publisher = {American Physical Society}, year = {2014}, volume = {90}, pages = {062712}, url = {http://link.aps.org/doi/10.1103/PhysRevA.90.062712}, doi = {10.1103/PhysRevA.90.062712} } 
"Plasma out of thermodynamical equilibrium : influence of the plasma environment on atomic structure and collisional cross sections" Belkhiri M, Thesis at: Université Paris XI  Paris Sud, (2014). 
Abstract: In hot dense plasmas, the interaction of an ion with other ions and free electrons may strongly affect the atomic structure. To account for such effects we have implemented a potential correction based on the uniform electron gas model and on a ThomasFermi Approach in the Flexible Atomic Code (FAC). This code has been applied to obtain energies, wavefunctions and radiative rates modified by the plasma environment. In hydrogenlike ions, these numerical results have been successfully compared to an analytical calculation based on firstorder perturbation theory. In the case of multielectron ions, we observe level crossings in agreement with another recent model calculation. Various methods for the collision crosssection calculations are reviewed. The influence of plasma environment on these crosssections is analyzed in detail. Some analytical expressions are proposed for hydrogenlike ions in the limit where Born or Lotz approximations apply and are compared to the numerical results from the FAC code. Finally, we study the influence of the plasma environment by including it in a new collisionalradiative model named Foch. Because of this environment, the mean charge state of the ions increases. The line shift is observed on the boundbound emission spectra. A good agreement is found between our work and experimental data on a Titanium plasma. 
BibTeX:
@phdthesis{Belkhiri2014, author = {Belkhiri, M.}, title = {Plasma out of thermodynamical equilibrium : influence of the plasma environment on atomic structure and collisional cross sections}, school = {Université Paris XI  Paris Sud}, year = {2014}, url = {http://www.theses.fr/2014PA112268} } 
"Linear response of a variational average atom in plasma: Semiclassical model " Caizergues C, Blenski T and Piron R, High Energy Density Physics. Vol. 12(0), pp. 12  20  (2014). 
Abstract: The frequencydependent linear response of a plasma is studied in the finitetemperature ThomaFermi approximation, with electron dynamics described using Bloch hydrodynamics. The variational framework of averageatoms in a plasma is used. Extinction crosssections are calculated for several plasma conditions. Comparisons with a previously studied ThomasFermi Impurity in Jellium model are presented. An Ehrenfesttype sum rule, originally proposed in a full quantum approach is derived in the present formalism and checked numerically. This sum rule is used to define Bremsstrahlung and collective contributions to the extinction crosssection. It is shown that none of these is negligible. Each can constitute the main contribution to the crosssection, depending on the frequency region and plasma conditions. This result obtained in the ThomasFermiBloch case stresses the importance of the selfconsistent approach to the linear response in general. Some of the methods used in this study can be extended to the linear response in the quantum case. 
BibTeX:
@article{Caizergues2014, author = {C. Caizergues and T. Blenski and R. Piron}, title = {Linear response of a variational average atom in plasma: Semiclassical model }, journal = {High Energy Density Physics }, year = {2014}, volume = {12}, number = {0}, pages = {12  20}, url = {http://www.sciencedirect.com/science/article/pii/S1574181814000299}, doi = {10.1016/j.hedp.2014.04.004} } 
2013 
"Iron and Nickel spectral opacity calculations in conditions relevant for pulsating stellar envelopes and experiments" Gilles D, TurckChièze S, Busquet M, Thais F, Loisel G, Piau L, Ducret J, Blenski T, Blancard C, Cossé P, Faussurier G, Gilleron F, Pain J, Porcherot Q, Guzik J, Kilcrease D, Magee N, Harris J, BastianiCeccotti S, Delahaye F et Zeippen C, EPJ Web of Conferences. Vol. 59, pp. 14003, (2013). 
Abstract: Seismology of stars is strongly developing. To address this question we have formed an international collaboration, OPAC, to perform specific experimental measurements, compare opacity calculations, and improve the opacity calculations in stellar codes [1]. We consider the following opacity codes: SCO, CASSANDRA, STA, OPAS, LEDCOP, OP, SCORCG. Their comparison has shown large differences for Fe and Ni in equivalent conditions of envelopes of type II supernova precursors, temperatures between 15 and 40 eV and densities of a few mg/cm^{3} [24]. LEDCOP, OPAS, SCORCG structure codes and STA give similar results and differ from OP ones for the lower temperatures and for spectral interval values [3]. In this work we discuss the role of Configuration Interaction (CI) and the influence of the number of used configurations. We present and include in the opacity code comparisons new HULLACv9 calculations [5, 6] that include full CI. To illustrate the importance of this effect we compare different CI approximations (modes) available in HULLACv9 [7]. These results are compared to previous predictions and to experimental data. Differences with OP results are discussed. 
BibTeX:
@article{Gilles2013, author = {Gilles, D. and TurckChièze, S. and Busquet, M. and Thais, F. and Loisel, G. and Piau, L. and Ducret, J.E. and Blenski, T. and Blancard, C. and Cossé, P. and Faussurier, G. and Gilleron, F. and Pain, J.C. and Porcherot, Q. and Guzik, J.A. and Kilcrease, D.P. and Magee, N.H. and Harris, J. and BastianiCeccotti, S. and Delahaye, F. and Zeippen, C.J}, title = {Iron and Nickel spectral opacity calculations in conditions relevant for pulsating stellar envelopes and experiments}, journal = {EPJ Web of Conferences}, year = {2013}, volume = {59}, pages = {14003}, url = {https://doi.org/10.1051/epjconf/20135914003}, doi = {10.1051/epjconf/20135914003} } 
"Theoretical interpretation for 2p  nd absorption spectra of iron, nickel, and copper in Xray range measured at the LULI2000 facility" Poirier M, Arnault P, BastianiCeccotti S, Blenski T, de Gaufridy de Dortan F, Gilleron F, Loisel G, Pain JC, Porcherot Q, Reverdin C, Silvert V, Thais F et TurckChièze S, EPJ Web of Conferences. Vol. 59, pp. 14001, (2013). 
Abstract: The 2p  nd absorption structures in medium Z elements present a valuable benchmark for atomic models since they exhibit a complex dependence on temperature and density. For these transitions lying in the Xray range, one observes a competition between the spinorbit splitting and the broadening associated to the excitation of complex structures. Detailed opacity codes based on the HULLAC or FAC suites agree with the statistical code SCO; but in iron computations predict higher peak absorption than measured. An addition procedure on opacities calculated with detailed codes is proposed and successfully tested. 
BibTeX:
@article{Poirier2013a, author = {Poirier, M. and Arnault, P. and BastianiCeccotti, S. and Blenski, T. and de Gaufridy de Dortan, F. and Gilleron, F. and Loisel, G. and Pain, J.C. and Porcherot, Q. and Reverdin, C. and Silvert, V. and Thais, F. and TurckChièze, S.}, title = {Theoretical interpretation for 2p  nd absorption spectra of iron, nickel, and copper in Xray range measured at the LULI2000 facility}, journal = {EPJ Web of Conferences}, year = {2013}, volume = {59}, pages = {14001}, url = {https://doi.org/10.1051/epjconf/20135914001}, doi = {10.1051/epjconf/20135914001} } 
"Models of atoms in plasmas based on common formalism for bound and free electrons " Blenski T, Piron R, Caizergues C and Cichocki B, High Energy Density Physics. Vol. 9(4), pp. 687  695  (2013). 
Abstract: Atominplasma models: ThomasFermi (TF) and INFERNO, AJCI and VAAQP, that use the same formalism for all electrons are briefly described and analyzed from the point of view of their thermodynamic consistence. While the TF and VAAQP models may be derived from variational principle and respect the virial theorem, it appears that two earlier quantum extensions of the quasiclassical TF model, INFERNO and AJCI, are not fully variational. The problems of the two latter approaches are analyzed from the point of view of the VAAQP model. However all quantum models seem to give unrealistic description of atoms in plasma at low temperature and high plasma densities. These difficulties are connected with the WignerSeitz cavity approach to noncentral ions that is present in all considered models. Comparison of some equationofstate data from TF, INFERNO and VAAQP models are shown on a chosen example. We report also on the status of our research on the frequencydependent linearresponse theory of atoms in plasma. A new Ehrenfesttype sum rule, originally proposed in the quantum VAAQP model, was proven in the case of the response of the TF atom with the Bloch hydrodynamics (TFB) and checked by numerical example. The TFB case allows one to have a direct insight into the rather involved mathematics of the selfconsistent linear response calculations in situations when both the central atom and its plasma vicinity are perturbed by an electric field. 
BibTeX:
@article{Blenski2013, author = {T. Blenski and R. Piron and C. Caizergues and B. Cichocki}, title = {Models of atoms in plasmas based on common formalism for bound and free electrons }, journal = {High Energy Density Physics }, year = {2013}, volume = {9}, number = {4}, pages = {687  695}, url = {http://www.sciencedirect.com/science/article/pii/S1574181813001493}, doi = {10.1016/j.hedp.2013.06.003} } 
"Variational AverageAtom in Quantum Plasmas (VAAQP)  Application to radiative properties", Piron R and Blenski T, High Energy Density Physics. Vol. 9(4), pp. 702  710  (2013). 
Abstract: We present an application of the Variational AverageAtom in Quantum Plasmas (VAAQP) model and numerical code to dense plasmas radiative properties. We propose an approximate Detailed Configuration Accounting (DCA) approach starting from the variational model of configurations in jellium. This leads to a simplified model which is qualitatively different from those which usually stem from the atomincell approach. It is also shown that, with some additional approximations, the DCA calculation can be handled by use of the Gaussian approximation to perform a statistical approach to the spectrum. Our purpose here is to show that this model provides a simple way to calculate the radiative properties and is likely to give realistic results. 
BibTeX:
@article{Piron2013, author = {R. Piron and T. Blenski}, title = {Variational AverageAtom in Quantum Plasmas (VAAQP) Ã¢â‚¬â€œ Application to radiative properties }, journal = {High Energy Density Physics }, year = {2013}, volume = {9}, number = {4}, pages = {702  710}, url = {http://www.sciencedirect.com/science/article/pii/S1574181813001626}, doi = {10.1016/j.hedp.2013.07.002} } 
"Density effects in plasmas: detailed atomic calculations and analytical expressions" Belkhiri M and Poirier M, High Energy Density Physics. Vol. 9(3), pp. 609617  (2013). 
Abstract: In warm dense plasmas, the freeelectron and ion spatial distribution may strongly affect atomic structure. To account for such effects we have implemented a potential correction based on uniform electron gas model in the Flexible Atomic Code. This code has been applied to get energies, wavefunctions and radiative rates modified by the plasma environment. In hydrogenlike ions, these numerical results have been successfully compared to an analytical calculation based on firstorder perturbation theory. In the case of multielectron ions, we observe level crossings in agreement with another recent model calculation. 
BibTeX:
@article{Belkhiri2013, author = {Belkhiri, M. and Poirier, M.}, title = {Density effects in plasmas: detailed atomic calculations and analytical expressions}, journal = {High Energy Density Physics}, year = {2013}, volume = {9}, number = {3}, pages = {609617}, url = {http://www.sciencedirect.com/science/article/pii/S1574181813000773}, doi = {10.1016/j.hedp.2013.05.016} } 
"Testing the reliability of nonLTE spectroscopic models for complex ions" Hansen S, Armstrong G, BastianiCeccotti S, Bowen C, HK C, Colgan J, de Gaufridy de Dortan F, Fontes C, Gilleron F, Marquès JR, Piron R, Peyrusse O, Poirier M, Ralchenko T, Sasaki A, Stambulchik E and Thais F, High Energy Density Physics. Vol. 9(3), pp. 523527  (2013). 
Abstract: Collisionalradiative atomic models are widely used to help diagnose experimental plasma conditions through fitting and interpreting measured spectra. Here we present the results of a code comparison in which a variety of models determined plasma temperatures and densities by finding the best fit to an experimental Lshell Kr spectrum from a well characterized, but not benchmarked, laser plasma. While variations in diagnostic strategies and qualities of fit were significant, the results generally confirmed the typically quoted uncertainties for such diagnostics of Â±20% in electron temperature and factors of about two in density. The comparison also highlighted some model features important for spectroscopic diagnostics: fine structure was required to match line positions and relative intensities within each charge state and for density diagnostics based on emission from metastable states; an extensive configuration set was required to fit the wings of satellite features and to reliably diagnose the temperature through the inferred charge state distribution; and the inclusion of selfconsistent opacity effects was an important factor in the quality of the fit. 
BibTeX:
@article{Hansen2013, author = {Hansen, S. and Armstrong, G.S.J. and BastianiCeccotti, S. and Bowen, C. and Chung HK and Colgan, J.P. and de Gaufridy de Dortan, F. and Fontes, C.J. and Gilleron, F. and Marquès, J.R. and Piron, R. and Peyrusse, O. and Poirier, M. and Ralchenko, Tu. and Sasaki, A. and Stambulchik, E. and Thais, F.}, title = {Testing the reliability of nonLTE spectroscopic models for complex ions}, journal = {High Energy Density Physics}, year = {2013}, volume = {9}, number = {3}, pages = {523527}, url = {http://www.sciencedirect.com/science/article/pii/S1574181813000633}, doi = {10.1016/j.hedp.2013.05.002} } 
"Analytical description of absorption profiles in warm dense plasmas: discussion of the nonoverlappingline limit" Poirier M, High Energy Density Physics. Vol. 9(3), pp. 618625  (2013). 
Abstract: This paper is devoted to a theoretical description of the spectral absorption in warm dense plasmas, such as those involved in hohlraumbased opacity measurements. Dealing with complex spectra, when the effect of natural and experimental broadening, optical thickness and line overlap is taken into account, the calculation of plasma transmission becomes quite elaborate. In the hypothesis of large experimental broadening, simple analytical formulas are obtained here for this transmission. They are checked by comparison to the exact convolution of various detailed spectra with a broadening profile. The current numerical method is then applied to the computation of transmission in Fe and Br plasmas, where opacity and lineoverlap effects may be substantial. 
BibTeX:
@article{Poirier2013, author = {Poirier, M.}, title = {Analytical description of absorption profiles in warm dense plasmas: discussion of the nonoverlappingline limit}, journal = {High Energy Density Physics}, year = {2013}, volume = {9}, number = {3}, pages = {618625}, url = {http://www.sciencedirect.com/science/article/pii/S1574181813000803}, doi = {10.1016/j.hedp.2013.05.019} } 
"Radiative properties of stellar envelopes: Comparison of asteroseismic results to opacity calculations and measurements for iron and nickel" TurckChièze S, Gilles D, Le Pennec M, Blenski T, Thais F, BastianiCeccotti S, Blancard C, Busquet M, Caillaud T, Colgan J, Cossé P, Delahaye F, Ducret JE, Faussurier G, Fontes C, Gilleron F, Guzik J, Harris J, Kilcrease D, Magee N, Pain J, Reverdin C, Silvert V, Villette B and Zeippen C, High Energy Density Physics. Vol. 9(3), pp. 473479  (2013). 
Abstract: The international OPAC consortium consists of astrophysicists, plasma physicists and experimentalists who examine opacity calculations used in stellar physics that appear questionable and perform new calculations and laser experiments to understand the differences and improve the calculations. We report on iron and nickel opacities for envelopes of stars from 2 to

BibTeX:
@article{TurckChieze2013, author = {TurckChièze, S. and Gilles, D. and Le Pennec, M. and Blenski, T.J. and Thais, F. and BastianiCeccotti, S. and Blancard, C. and Busquet, M. and Caillaud, T. and Colgan, J. and Cossé, P. and Delahaye, F. and Ducret, J.E. and Faussurier, G. and Fontes, C.J. and Gilleron, F. and Guzik, J. and Harris, J. and Kilcrease, D.P. and Magee, N.H. and Pain, J.C. and Reverdin, C. and Silvert, V. and Villette, B. and Zeippen, C.J.}, title = {Radiative properties of stellar envelopes: Comparison of asteroseismic results to opacity calculations and measurements for iron and nickel}, journal = {High Energy Density Physics}, year = {2013}, volume = {9}, number = {3}, pages = {473479}, url = {http://www.sciencedirect.com/science/article/pii/S157418181300044X}, doi = {10.1016/j.hedp.2013.04.004} } 
"Optically Aligned, Space Resolving, Extreme UltraViolet and Soft Xray Spectrograph" Busquet M, Thais F, Geoffroy G, Raffestin D and Chièze J, Applied Physics Research. Vol. 5, pp. 2532  (2013). 
Abstract: We describe in this paper an extreme ultraviolet/soft Xray (XUV) spectrograph with high sensitivity, high spectral resolution and spatial resolution, which we developed to record XUV emission from a 10 J laserirradiated gas jet. This spectrograph uses a flat field grazing incidence grating and a grazing incidencecollection and imaging mirror. We designed a system where initial positions of elements can be set with a low accuracy of half a millimeter and where the final alignment is done with a visible light low intensity laser beam. High spectral resolution, good spatial resolution and nominal dispersion function have been achieved. A few illustrative results are presented. 
BibTeX:
@article{Busquet2013, author = {Busquet, M. and Thais, F. and Geoffroy, G. and Raffestin, D. and Chièze, J.P.}, title = {Optically Aligned, Space Resolving, Extreme UltraViolet and Soft Xray Spectrograph}, journal = {Applied Physics Research}, year = {2013}, volume = {5}, pages = {2532}, url = {http://dx.doi.org/10.5539/apr.v5n2p25} } 
2012 
"Velocity asymmetries in young stellar object jetsIntrinsic and extrinsic mechanisms" Matsakos T, Vlahakis N, Tsinganos K, Karampelas K, Sauty C, Cayatte V, Matt S, Massaglia S, Trussoni E and Mignone A, Astronomy and Astrophysics. Vol. 545, pp. A53  (2012). 
Abstract: Context. It is well established that some YSO jets (e.g. RW Aur) display different propagation speeds between their blue and redshifted parts, a feature possibly associated with the central engine or the environment in which the jet propagates.Aims. To understand the origin of asymmetric YSO jet velocities, we investigate the efficiency of two candidate mechanisms, onebased on the intrinsic properties of the system and the other on the role of the external medium. In particular, a parallel or antiparallelconfiguration between the protostellar magnetosphere and the disk magnetic field is considered, and the resulting dynamics examinedboth in an ideal and in a resistive magnetohydrodynamical (MHD) regime. Moreover, we explore the effects of a potential differencein the pressure of the environment, as a consequence of the nonuniform density distribution of molecular clouds.Methods. Ideal and resistive axisymmetric numerical simulations were carried out for a variety of models, all of which are basedon a combination of two analytical solutions, a disk wind and a stellar outflow. The initial twocomponent jet is modified by eitherinverting the orientation of its inner magnetic field or imposing a constant surrounding pressure. The velocity profiles are studied byassuming steady flows as well as after strong time variable ejection is incorporated.Results. Discrepancies between the speeds of the two outflows in opposite directions can indeed occur both due to unaligned magneticfields and different outer pressures. In the former case, the asymmetry appears only on the dependence of the velocity on the cylindricaldistance, but the implied observed value is significantly altered when the density distribution is also taken into account. On the otherhand, a nonuniform medium collimates the two jets unevenly, directly affecting their propagation speed. A further interesting featureof the pressureconfined outflow simulations is the formation of static knots whose spacing seems to be associated with the ambientpressure.Conclusions. Jet velocity asymmetries are anticipated both when multipolar magnetic moments are present in the stardisk systemand when nonuniform environments are considered. The latter is an external mechanism that can easily explain the large timescale ofthe phenomenon, whereas the former naturally relates it to the YSO intrinsic properties. 
BibTeX:
@article{Matsakos2012, author = {Matsakos, T. and Vlahakis, N. and Tsinganos, K. and Karampelas, K. and Sauty, C. and Cayatte, V. and Matt, S.P. and Massaglia, S. and Trussoni, E. and Mignone, A.}, title = {Velocity asymmetries in young stellar object jetsIntrinsic and extrinsic mechanisms}, journal = {Astronomy and Astrophysics}, year = {2012}, volume = {545}, pages = {A53}, url = {http://dx.doi.org/10.1051/00046361/201219498}, doi = {10.1051/00046361/201219498} } 
"Equation of State of Dense Plasma Mixtures: Application to the Sun Center" Pain J, Dejonghe G and Blenski T, Contribution to Plasma Physics. Vol. 52, pp. 2327  (2012). 
Abstract: We present a selfconsistent approach to the modeling of dense plasma mixtures in local thermodynamic equilibrium. In each electron configuration the nucleus is totally screened by electrons in a WignerSeitz sphere (ionsphere model). Bound and free electrons are treated quantummechanically. The assumption that all species should have the same electronic environment leads to the equality of the electronic pressure for all ions of all elements having therefore different cell volumes. The variation of the average atomic radii of the different elements with respect to temperature is investigated, and the procedure is applied to the determination of pressure in the Sun center 
BibTeX:
@article{Pain2012, author = {Pain, J.C. and Dejonghe, G. and Blenski, T.}, title = {Equation of State of Dense Plasma Mixtures: Application to the Sun Center}, journal = {Contribution to Plasma Physics}, year = {2012}, volume = {52}, pages = {2327}, url = {http://dx.doi.org/10.1002/ctpp.201100069} } 
"Xray grating spectrometer for opacity measurements in the 50 eV to 250 eV spectral range at the LULI 2000 laser facility" Reverdin C, Thais F, Loisel G, Busquet M, BastianiCeccotti S, Blenski T, Caillaud T, Ducret J, Foelsner W, Gilles D, Gilleron F, Pain J, Poirier M, Serres F, Silvert V, Soullie G, TurckChièze S and Villette B, Review of Scientific Instruments. Vol. 83, pp. 10E134  (2012). 
Abstract: An xray grating spectrometer was built in order to measure opacities in the 50 eV to 250 eV spectral range with an average spectral resolution (E/dE) ~ 50. It has been used at the LULI2000 laser facility at école Polytechnique (France) to measure the ?n = 0, n = 3 transitions of several elements with neighboring atomic number: Cr, Fe, Ni, and Cu in the same experimental conditions. Hence a spectrometer with a wide spectral range is required. This spectrometer features one line of sight looking through a heated sample at backlighter emission. It is outfitted with one toroidal condensing mirror and several flat mirrors cutting off higher energy photons. The spectral dispersion is obtained with a flatfield grating. Detection consists of a streak camera sensitive to soft xray radiation. Some experimental results showing the performance of this spectrometer are presented. 
BibTeX:
@article{Reverdin2012, author = {Reverdin, C. and Thais, F. and Loisel, G. and Busquet, M. and BastianiCeccotti, S. and Blenski, T. and Caillaud, T. and Ducret, J.E. and Foelsner, W. and Gilles, D. and Gilleron, F. and Pain, J.C. and Poirier, M. and Serres, F. and Silvert, V. and Soullie, G. and TurckChièze, S. and Villette, B.}, title = {Xray grating spectrometer for opacity measurements in the 50 eV to 250 eV spectral range at the LULI 2000 laser facilit}, journal = {Review of Scientific Instruments}, year = {2012}, volume = {83}, pages = {10E134}, url = {http://link.aip.org/link/?RSI/83/10E134}, doi = {10.1063/1.4740266} } 
"Counterrotation in magnetocentrifugally driven jets and other winds" Sauty C, Cayatte V, Lima J, Matsakos T and Tsinganos K, Astrophysical Journal Letters, The. Vol. 759, pp. L1  (2012). 
Abstract: Rotationmeasurements in jets from T Tauri stars is a rather difficult task. Some jets seem to be rotating in a direction opposite to that of the underlying disk, although it is not yet clear if this affects the totality or part of the utflows. On the other hand, Ulysses data also suggest that the solar wind may rotate in two opposite ways between the northern and southern hemispheres. We show that this result is not surprising as it may seem and that it emerges naturally from the ideal MHD equations. Specifically, counterrotating jets do not contradict the magnetocentrifugal driving of the flow nor prevent extraction of angular momentum from the disk. The demonstration of this result is shown by combining the ideal MHD equations for steady axisymmetric flows. Provided that the jet is decelerated below some given threshold beyond the AlfvÂ´en surface, the flow will change its direction of rotation locally or globally. Counterrotation is also possible for only some layers of the outflow at specific altitudes along the jet axis. We conclude that the counterrotation of winds or jets with respect to the source, star or disk, is not in contradiction with the magnetocentrifugal driving paradigm. This phenomenon may affect part of the outflow, either in one hemisphere, or only in some of the outflow layers. From a timedependent simulation, we illustrate this effect and show that it may not be permanent. 
BibTeX:
@article{Sauty2012, author = {Sauty, C. and Cayatte, V. and Lima, J.J.G. and Matsakos, T. and Tsinganos, K.}, title = {Counterrotation in magnetocentrifugally driven jets and other winds}, journal = {Astrophysical Journal Letters, The}, year = {2012}, volume = {759}, pages = {L1}, url = {http://iopscience.iop.org/20418205/759/1/L1/}, doi = {10.1088/20418205/759/1/L1} } 
2011 
"Electronhole dynamics in normal and deuterated KH2PO4 illuminated by intense femtosecond laser pulses" Duchateau G, Geoffroy G, Dyan A, Piombini H and Guizard S, Physical Review B. Vol. 83(7), pp. 075114\_111  (2011). 
Abstract: The dynamics of electrons and holes in potassium dihydrogen phosphate (KH_{2}PO_{4} or KDP) crystals and its deuterated analog (KD_{2}PO_{4} or DKDP) induced by femtosecond laser pulses is investigated at λ=800 nm. To do so, experiments based on a femtosecond timeresolved interferometry technique have been carried out. It is shown that two relaxation dynamics exist in KDP and DKDP crystals. Both of them correspond to physical mechanisms for which the multiphoton order required to promote valence electrons to the conduction band is lower than the one of a defectfree crystal. These results suggest the presence of states located in the band gap that may be due to the presence of defects existing before any laser illumination or created in the course of interaction. In order to interpret the experiments, a model based on a kinetic equation system has been developed. Modeling results are in good agreement with the experimental data. 
BibTeX:
@article{Duchateau2011, author = {Duchateau, G. and Geoffroy, G. and Dyan, A. and Piombini, H. and Guizard, S.}, title = {Electronhole dynamics in normal and deuterated KH2PO4 illuminated by intense femtosecond laser pulses}, journal = {Physical Review B}, year = {2011}, volume = {83}, number = {7}, pages = {075114111}, url = {http://prb.aps.org/abstract/PRB/v83/i7/e075114}, doi = {10.1103/PhysRevB.83.075114} } 
"Theoretical interpretation of Xrays photoabsorption in mediumZ elements plasmas measured at LULI2000 facility" Blenski T, Loisel G, Poirier M, Thais F, Arnault P, Caillaud T, Fariaut J, Gilleron F, Pain JC, Porcherot Q, Reverdin C, Silvert V, Villette B, BastianiCeccotti S, TurckChièze S, Foelsner W and de Gaufridy de Dortan F, High Energy Density Physics. Vol. 7(4), pp. 320326  (2011). 
Abstract: We analyzed the spectra of Xray transmission through radiatively heated mediumZ plasma (Fe, Ni, Cu and Ge) measured at LULI2000 facility in the wavelength range of 2pâ€“nd transitions. The analysis was performed using the statistical superconfiguration code SCO, two linebyline opacity codes based on the HULLAC and FAC packages and a new hybrid statisticaldetailed code SCORCG. The temperature and mass density of the samples were estimated from hydrodynamic simulations based on the cavity radiative temperature measurements. The theoryâ€“experiment agreement is relatively good in the wavelength range corresponding to the 2pâ€“3d transitions except in the germanium case. In the wavelength range of the 2pâ€“2d, n > 3 transitions a relatively good theoryâ€“experiment agreement was found in the copper case. As predicted by calculations the separation of the characteristic spinorbitsplit 2pâ€“3d structures, absent in the iron measured spectrum, appears in the nickel spectrum and is visible in the copper and germanium spectra. Comparisons of the experimental transmission with calculations confirm the importance of the relativistic configuration interaction. The absorption strength of the measured germanium 2pâ€“3d transition is much larger than that obtained from the codes. Spatial temperature and density gradients, relatively high in the germanium sample, may be at the origin of this discrepancy. 
BibTeX:
@article{Blenski2011, author = {Blenski, T.J. and Loisel, G. and Poirier, M. and Thais, F. and Arnault, P. and Caillaud, T. and Fariaut, J. and Gilleron, F. and Pain, J.C. and Porcherot, Q. and Reverdin, C. and Silvert, V. and Villette, B. and BastianiCeccotti, S. and TurckChièze, S. and Foelsner, W. and de Gaufridy de Dortan, F.}, title = {Theoretical interpretation of Xrays photoabsorption in mediumZ elements plasmas measured at LULI2000 facility}, journal = {High Energy Density Physics}, year = {2011}, volume = {7}, number = {4}, pages = {320326}, url = {http://www.sciencedirect.com/science/article/pii/S1574181811000759}, doi = {10.1016/j.hedp.2011.06.006} } 
"Opacity of iron, nickel and copper plasmas in the xray wavelength range: theoretical interpretation of 2p  3d absorption spectra" Blenski T, Loisel G, Poirier M, Thais F, Arnault P, Caillaud T, Fariaut J, Gilleron F, Pain JC, Porcherot Q, Reverdin C, Silvert V, Villette B, BastianiCeccotti S, TurckChieze S, Folsner W and de Gaufridy de Dortan F, Physical Review E  Statistical, Nonlinear and Soft Matter Physics. Vol. 84, pp. 036407_117  (2011). 
Abstract: This paper deals with theoretical studies on the 2p3d absorption in iron, nickel, and copper plasmas related to LULI2000 (Laboratoire pour l'Utilisation des Lasers Intenses, 2000J facility) measurements in which target temperatures were of the order of 20 eV and plasma densities were in the range 0.004â€“0.01 g/cm3. The radiatively heated targets were close to local thermodynamic equilibrium (LTE). The structure of 2p3d transitions has been studied with the help of the statistical superconfiguration opacity code sco and with the finestructure atomic physics codes hullac and fac. A new mixed version of the sco code allowing one to treat part of the configurations by detailed calculation based on the Cowan's code rcg has been also used in these comparisons. Special attention was paid to comparisons between theory and experiment concerning the term features which cannot be reproduced by sco. The differences in the spinorbit splitting and the statistical (thermal) broadening of the 2p3d transitions have been investigated as a function of the atomic number Z. It appears that at the conditions of the experiment the role of the term and configuration broadening was different in the three analyzed elements, this broadening being sensitive to the atomic number. Some effects of the temperature gradients and possible nonLTE effects have been studied with the help of the radiativecollisional code scric. The sensitivity of the 2p3d structures with respect to temperature and density in mediumZ plasmas may be helpful for diagnostics of LTE plasmas especially in future experiments on the ?n=0 absorption in mediumZ plasmas for astrophysical applications. 
BibTeX:
@article{Blenski2011a, author = {Blenski, T.J. and Loisel, G. and Poirier, M. and Thais, F. and Arnault, P. and Caillaud, T. and Fariaut, J. and Gilleron, F. and Pain, J.C. and Porcherot, Q. and Reverdin, C. and Silvert, V. and Villette, B. and BastianiCeccotti, S. and TurckChieze, S. and Folsner, W. and de Gaufridy de Dortan, F.}, title = {Opacity of iron, nickel and copper plasmas in the xray wavelength range: theoretical interpretation of 2p  3d absorption spectra}, journal = {Physical Review E  Statistical, Nonlinear and Soft Matter Physics}, year = {2011}, volume = {84}, pages = {036407_117}, url = {http://dx.doi.org/10.1103/PhysRevE.84.036407}, doi = {10.1103/PhysRevE.84.036407} } 
"On the influence of opacity variation on spatial structure of radiative shocks" Busquet M, Klapisch M and Thais F, High Energy Density Physics. Vol. 7(4), pp. 217223  (2011). 
Abstract: We provide a theoretical analysis of Radiative Shocks, defined as supercritical shocks accompanied by an ionization wave in front of the density jump. In particular, we look at the influence of opacity variation with temperature and photon energy on spatial structure of radiative shocks, with a view to understanding a split precursor feature observed in recent experiments. We show that multigroup processing, a more refined angular description and improved low temperature opacities are needed to explore the radiative precursor structure, at least in some temperature regimes where rapid change of ionization can be found. 
BibTeX:
@article{Busquet2011, author = {Busquet, M. and Klapisch, M. and Thais, F.}, title = {On the influence of opacity variation on spatial structure of radiative shocks}, journal = {High Energy Density Physics}, year = {2011}, volume = {7}, number = {4}, pages = {217223}, url = {http://www.sciencedirect.com/science/article/pii/S1574181811000516}, doi = {10.1016/j.hedp.2011.04.010} } 
"Comparison of Fe and Ni opacity calculations for a better understanding of pulsating stellar envelopes" Gilles D, TurckChieze S, Loisel G, Piau L, Ducret JE, Blenski T, Poirier M, Thais F, Blancard C, Cossé P, Faussurier G, Gilleron F, Pain JC, Porcherot Q, Guzik J, Kilcrease D, Magee N, Harris J, Busquet M, Delahaye F, Zeippen C and BastianiCeccotti S, High Energy Density Physics. Vol. 7(4), pp. 312319 (2011). 
Abstract: Opacity is an important ingredient of the secular evolution of stars. The calculation of opacity coefficients is complex because the plasma is generally partially ionized for the heavy ions contribution of a mixture dominated by H/He. Up to now, the astrophysical community has greatly benefited from the work of the Los Alamos and OPAL teams and also from the Opacity Project (OP) tables and their corresponding spectra. However unexplained differences in the radiative forces and Rosseland mean values for Fe up to 50% have been noticed for conditions corresponding to stellar envelopes. Such uncertainty has a real impact on the understanding of pulsating stellar envelopes on the excitation of modes and on the identification of the mode frequencies. Temperature and density conditions equivalent to those found in stars can now be produced in laboratory experiments for different atomic species. Recently the photoabsorption spectra of nickel and iron plasmas have been measured during the LULI 2010 campaign, for temperatures between 15 and 40 eV and densities of ~3 mg/cm3. A large theoretical collaboration (consortium "OPAC") has been formed to prepare this experiment. We present here the panel of opacity calculations performed by eight different groups for conditions relevant to the LULI 2010 experiment and to astrophysical stellar envelope conditions. 
BibTeX:
@article{Gilles2011, author = {Gilles, D. and TurckChieze, S. and Loisel, G. and Piau, L. and Ducret, J.E. and Blenski, T.J. and Poirier, M. and Thais, F. and Blancard, C. and Cossé, P. and Faussurier, G. and Gilleron, F. and Pain, J.C. and Porcherot, Q. and Guzik, J.A. and Kilcrease, D.P. and Magee, N.H. and Harris, J. and Busquet, M. and Delahaye, F. and Zeippen, C.J. and BastianiCeccotti, S.}, title = {Comparison of Fe and Ni opacity calculations for a better understanding of pulsating stellar envelopes}, journal = {High Energy Density Physics}, year = {2011}, volume = {7}, number = {4}, pages = {312319}, url = {http://www.sciencedirect.com/science/article/pii/S1574181811000723}, doi = {10.1016/j.hedp.2011.06.001} } 
"Variational AverageAtom in Quantum Plasmas (VAAQP) Recent progress, virial theorem and applications to the equationofstate of warm dense Be" Piron R and Blenski T, High Energy Density Physics. Vol. 7, pp. 346352  (2011). 
Abstract: The Variational AverageAtom in Quantum Plasmas (VAAQP) code is based on a fully variational theory of dense plasmas in equilibrium in which the neutrality of the WignerSeitz ion sphere is not required, contrary to the Inferno model. We report on some recent progress in the VAAQP model and numerical code. Three important points of the virial theorem derivation are emphasized and explained. The virial theorem is also used as an important tool allowing us to check the formulas and numerical methods used in the code. Applications of the VAAQP code are shown using as an example the equationofstate of beryllium in the warm dense matter regime. Comparisons with the Inferno model, and with available experimental data on the principal Hugoniot are also presented. 
BibTeX:
@article{Piron2011, author = {Piron, R. and Blenski, T.}, title = {Variational AverageAtom in Quantum Plasmas (VAAQP) Recent progress, virial theorem and applications to the equationofstate of warm dense Be}, journal = {High Energy Density Physics}, year = {2011}, volume = {7}, pages = {346352}, url = {http://dx.doi.org/10.1016/j.hedp.2011.06.006}, doi = {10.1016/j.hedp.2011.06.006} } 
"Variationalaverageatominquantumplasmas (VAAQP) code and virial theorem: Equationofstate and shockHugoniot calculations for warm dense Al, Fe, Cu, and Pb" Piron R and Blenski T, Physical Review E  Statistical, Nonlinear and Soft Matter Physics. Vol. 83, pp. 026403_122  (2011). 
Abstract: A numerical code: VAAQP (Variational AverageAtom in Quantum Plasmas) which is based on a fully variational model of equilibrium dense plasmas is applied to equationofstate calculations for aluminum, iron, copper and lead in the warm dense matter regime. VAAQP does not impose the neutrality of the WignerSeitz ion sphere, it provides the averageatom structure and the mean ionization selfconsistently from the solution of the variational equations. The formula used for the electronic pressure is simple and does not require any numerical differentiation. In this article, the virial theorem is derived in both nonrelativistic and relativistic versions of the model. This theorem allows one to express the electron pressure as a combination of the electron kinetic and interaction energies. It is shown that the model fulfills automatically the virial theorem in case of local density approximations to the exchangecorrelation free energy. Applications of the model to the equationofstate and Hugoniot shock adiabat of aluminum, iron, copper and lead in the warm dense matter regime are presented. Comparisons with other approaches, including the INFERNO model, and with available experimental data are given. This work allows one to understand the thermodynamic consistency issues in the existing averageatom models. Starting from the case of aluminum, a comparative study of the thermodynamic consistency of the models is proposed. A preliminary study of the validity domain of the INFERNO model is also included. 
BibTeX:
@article{Piron2011a, author = {Piron, R. and Blenski, T.J.}, title = {Variationalaverageatominquantumplasmas (VAAQP) code and virial theorem: Equationofstate and shockHugoniot calculations for warm dense Al, Fe, Cu, and Pb}, journal = {Physical Review E  Statistical, Nonlinear and Soft Matter Physics}, year = {2011}, volume = {83}, pages = {026403_122}, url = {http://link.aps.org/doi/10.1103/PhysRevE.83.026403}, doi = {10.1103/PhysRevE.83.026403} } 
"A consistent approach for mixed detailed and statistical calculation of opacities in hot plasmas" Porcherot Q, Pain JC, Gilleron F and Blenski T, High Energy Density Physics. Vol. 7(4), pp. 234239  (2011). 
Abstract: Absorption and emission spectra of plasmas with multichargedions contain transition arrays with a huge number of coalescent electricdipole (E1) lines, which are well suited for treatment by the unresolved transition array and derivative methods. But, some transition arrays show detailed features whose description requires diagonalization of the Hamiltonian matrix. We developed a hybrid opacity code, called SCORCG, which combines statistical approaches with finestructure calculations consistently. Data required for the computation of detailed transition arrays (atomic configurations and atomic radial integrals) are calculated by the superconfiguration code SCO (SuperConfiguration Opacity), which provides an accurate description of the plasma screening effects on the wavefunctions. Level energies as well as position and strength of spectral lines are computed by an adapted RCG routine of R. D. Cowan. The resulting code provides opacities for hot plasmas and can handle midZ elements. The code is also a powerful tool for the interpretation of recent laser and Zpinch experimental spectra, as well as for validation of statistical methods. 
BibTeX:
@article{Porcherot2011, author = {Porcherot, Q. and Pain, J.C. and Gilleron, F. and Blenski, T.J.}, title = {A consistent approach for mixed detailed and statistical calculation of opacities in hot plasmas}, journal = {High Energy Density Physics}, year = {2011}, volume = {7}, number = {4}, pages = {234239}, url = {http://www.sciencedirect.com/science/article/pii/S1574181811000528}, doi = {10.1016/j.hedp.2011.05.001} } 
"Radiative properties of stellar plasmas and open challenges" TurckChièze S, Loisel G, Gilles D, Piau L, Blancard C, Blenski T, Busquet M, Cosse P, Delahaye F, Faussurier G, Gilleron F, Guzik J, Harris J, Kilcrease D, Magee N, Pain J, Porcherot Q, Poirier M, Zeippen C, BastianiCeccotti S, Reverdin C, Silvert V and Thais F, Astrophysics and Space Science. Vol. 336, pp. 103109  (2011). 
Abstract: The lifetime of solarlike stars, the envelopof more massive stars and the acoustic frequencieslargely depend on the radiative properties of the stellar plasmas. Up to now, these complex quantities have been estimated only theoretically. With the strong development of helio and astero seismology, a real insight on the stellar interiors is becoming a very active astrophysical research. Consequently, an increase pressure is put on the appropriate knowledge of the monochromatic opacity coefficients. In this review, we recall how these ingredients play a role and where the radiative properties are the most important to know. We then specifically concentrate on the envelops of the beta Cephei. We discuss the dispersion of eight different theoretical estimates of the monochromatic opacity spectrum and the challenges we need to face to check these calculations experimentally. 
BibTeX:
@article{TurckChieze2011a, author = {TurckChièze, S. and Loisel, G. and Gilles, D. and Piau, L. and Blancard, C. and Blenski, T.J. and Busquet, M. and Cosse, P. and Delahaye, F. and Faussurier, G. and Gilleron, F. and Guzik, J. and Harris, J. and Kilcrease, D.P. and Magee, N.H. and Pain, J.C. and Porcherot, Q. and Poirier, M. and Zeippen, C. and BastianiCeccotti, S. and Reverdin, C. and Silvert, V. and Thais, F.}, title = {Radiative properties of stellar plasmas and open challenges}, journal = {Astrophysics and Space Science}, year = {2011}, volume = {336}, pages = {103109}, url = {http://dx.doi.org/10.1007/s1050901005838}, doi = {10.1007/s1050901005838} } 
"Theoretical and experimental activities on opacities for a good interpretation of seismic stellar probes" TurckChièze S, Loisel G, Gilles D, Thais F, Bastiani S, Blancard C, Busquet M, Caillaud T, Cossé P, Blenski T, Delahaye F, Ducret J, Faussurier G, Gilleron F, Guzik J, Harris J, Kilcrease D, Magee N, Piau L, Pain J, Poirier M, Porcherot Q, Reverdin C, Silvert V, Villette B and Zeippen C, Journal of Physics Conference Series. Vol. 271, pp. 012035  (2011). 
Abstract: Opacity calculations are basic ingredients of stellar modelling. They play a crucial role in the interpretation of acoustic modes detected by SoHO, COROT and KEPLER. In this review we present our activities on both theoretical and experimental sides. We show new calculations of opacity spectra and comparisons between eight groups who produce opacity spectra calculations in the domain where experiments are scheduled. Real differences are noticed with real astrophysical consequences when one extends helioseismology to cluster studies of different compositions. Two cases are considered presently: (1) the solar radiative zone and (2) the beta Cephei envelops. We describe how our experiments are performed and new preliminary results on nickel obtained in the campaign 2010 at LULI 2000 at Polytechnique. 
BibTeX:
@article{TurckChieze2011, author = {TurckChièze, S. and Loisel, G. and Gilles, D. and Thais, F. and Bastiani, S. and Blancard, C. and Busquet, M. and Caillaud, T. and Cossé, P. and Blenski, T.J. and Delahaye, F. and Ducret, J.E. and Faussurier, G. and Gilleron, F. and Guzik, J. and Harris, J.W. and Kilcrease, D.P. and Magee, N.H. and Piau, L. and Pain, J.C. and Poirier, M. and Porcherot, Q. and Reverdin, C. and Silvert, V. and Villette, B. and Zeippen, C.}, title = {Theoretical and experimental activities on opacities for a good interpretation of seismic stellar probes}, journal = {Journal of Physics Conference Series}, year = {2011}, volume = {271}, pages = {012035}, url = {http://dx.doi.org/10.1088/17426596/271/1/012035}, doi = {10.1088/17426596/271/1/012035} } 
"Des plasmas stellaires aux plasmas de laboratoire :Application aux mesures d'opacité dans les domainesX et XUV" Loisel G, In Astrophysique et physique des plasmas. Thesis at: Université Paris XI  Paris Sud, UFR Orsay (2011). 
Abstract: Cette thèse s'inscrit dans le contexte général des propriétés radiatives de la matière à haute densité d'énergie (>10^11 J/cm3). Les densités d'énergie de la MHDE font qu'une partie importante des échanges d'énergie passe par l'interaction rayonnementmatière. Mes études portent sur l'opacité spectrale, un paramètre fondamental pour la modélisation des intérieurs stellaires et qui constitue aussi une observable propice aux tests expérimentaux des descriptions théoriques de la physique des plasmas chauds et denses.Mes travaux de thèse sont centrés sur l'étude expérimentale des opacités de plasmas à l'équilibre thermodynamique local pour des températures de quelques dizaines d'eV (soit quelques 100 000 K) et quelques mg/cm3 en densité. Les plasmas sont obtenus dans des conditions aussi homogènes que possible en utilisant le chauffage radiatif d'une cavité irradiée par laser de haute énergie, 100300 J. Ainsi, nous avons pu mettre à profit pour ce type de mesure la configuration utilisant des lasers nanoseconde et picoseconde du LULI (Laboratoire pour l'Utilisation des Lasers Intenses) pour réaliser le chauffage d'une part et la mesure sur un temps bref d'autre part de la transmission des plasmas, l'utilisation d'impulsions courtes constituant une première pour ce type d'expériences.Dans le domaine des X de l'ordre du keV, les transitions absorbantes 2p3d ou 3d4f d'éléments de numéro atomique moyen ou élevé ont été sondées. Elles font apparaitre des structures d'absorption dont la forme résulte principalement de la compétition entre l'éclatement spinorbite et les effets d'élargissement statistiques. Il a été montré que cette compétition dépendait fortement du numéro atomique Z. Ainsi à paramètres plasma proches nous avons exploré l'opacité des éléments fer, nickel, cuivre et germanium (Z autour de 30) dans une première série de mesures puis celle du baryum, samarium et du gadolinium, dans une seconde expérience (Z autour de 60).L'astrophysique stellaire nécessite aussi de mesurer précisément, et de manière bien caractérisée, les opacités du groupe du fer (Cr, Fe, Ni et Cu) dans le domaine des XUV (50  200 eV). Ces opacités sont à l'origine de l'excitation dans les enveloppes radiatives des étoiles pulsantes massives de type spectral B pour une température de l'ordre de 200 000 K. Dans ces conditions, les moyennes de Rosseland présentent des différences nettes entre les calculs utilisés par la communauté astrophysique et ne permettent pas d'interpréter les oscillations et l'ensemble des fréquences observées de manière univoque. Pour permettre des comparaisons avec divers calculs spectraux, j'ai participé à la mise en place d'un nouveau schéma expérimental à deux cavités dont le but était d'améliorer l'homogénéité du chauffage des échantillons. Je montrerai enfin l'analyse des paramètres plasmas pour ce type de schéma. J'ai en particulier analysé le cas du nickel dont la transmission a été mesurée pour la première fois dans cette gamme spectrale.Dans chaque cas je présenterai l'analyse des résultats obtenus. 
BibTeX:
@phdthesis{PhdThesisLoisel2011, author = {Loisel, G.}, title = {Des plasmas stellaires aux plasmas de laboratoire :Application aux mesures d'opacité dans les domainesX et XUV}, booktitle = {Astrophysique et physique des plasmas}, school = {Université Paris XI  Paris Sud, UFR Orsay}, year = {2011}, url = {http://tel.archivesouvertes.fr/tel00579800/fr/} } 
2010 
"Relaxation dynamics of electronic excitations in CaWO4 and CdWO4 crystals studied by femtosecond interferometry technique" Nagirnyi V, Geoffroy G, Grigonis R, Guizard S, Kirm M, Kotlov A, Nagornaya L, Nikl M, Sirutkaitis V and Vielhauer S, Radiation Measurements. Vol. 45(36), pp. 262264  (2010). 
Abstract: The relaxation of electronic excitations in CdWO_{4} and CaWO_{4} crystals was studied using the method of timeresolved interferometry with 100fs temporal resolution at temperatures 15295 K. The electronic system was excited in the onephoton and twophoton regime within the excitonic band in CaWO_{4} and in the electronhole continuum in CdWO_{4}. Immediate trapping of charge carriers was detected under pumping in the excitonic band of CaWO_{4}. This result is in agreement with decay kinetics measurements with nanosecond time resolution under direct creation of excitons by 100fs laser pulses. Fast relaxation of charge carriers followed by formation of excitons was observed in CdWO_{4}. The comparison with previous work allows suggesting the formation of bulk excitons and surfaceperturbed excitons in the multiphoton and onephoton regime. The corresponding models of selftrapped exciton creation in tungstate crystals are discussed. 
BibTeX:
@article{Nagirnyi2010, author = {Nagirnyi, V. and Geoffroy, G. and Grigonis, R. and Guizard, S. and Kirm, M. and Kotlov, A. and Nagornaya, L.L. and Nikl, M. and Sirutkaitis, V. and Vielhauer, S.}, title = {Relaxation dynamics of electronic excitations in CaWO4 and CdWO4 crystals studied by femtosecond interferometry technique}, journal = {Radiation Measurements}, year = {2010}, volume = {45}, number = {36}, pages = {262264}, url = {http://www.sciencedirect.com/science/article/pii/S1350448709003746}, doi = {10.1016/j.radmeas.2009.12.007} } 
"Electron heating through a set of random levels in the conduction band of insulators induced by femtosecond laser pulses" Bachau H, Belsky A, Bogatyrev I, Gaudin J, Geoffroy G, Guizard S, Martin P, Popov YV, Vasil'ev A and Yatsenko B, Applied Physics A : Materials Science & Processing. Vol. 98, pp. 679689  (2010). 
Abstract: We develop a theory describing the heating ofelectrons in crystalline insulators irradiated by highintensitylaser pulses. In agreement with photoelectron yield versus intensity measurements, we assume that electrons are excited into the conduction band from defect layers and traps.The electron dynamics due to direct interbranch transitions within the conduction band is simulated by solving of timedependent Schrodinger equation. The set of levels for this equation is supposed to be random with a distribution function equal to the density of states in the conduction band.The influence of different parameters on the electron heating efficiency is studied. The theory is applied for diamond; the theoretical spectrum is in qualitative agreement with the experimental observations. 
BibTeX:
@article{Bachau2010, author = {Bachau, H. and Belsky, A. and Bogatyrev, I.B. and Gaudin, J. and Geoffroy, G. and Guizard, S. and Martin, P. and Popov, Yu. V. and Vasil'ev, A.N. and Yatsenko, B.N.}, title = {Electron heating through a set of random levels in the conduction band of insulators induced by femtosecond laser pulses}, journal = {Applied Physics A : Materials Science & Processing}, year = {2010}, volume = {98}, pages = {679689}, url = {http://link.springer.com/article/10.1007%2Fs003390095465y}, doi = {10.1007/s003390095465y} } 
"Measure of precursor electron density profiles of laser launched radiative shocks" Busquet M, Thais F, Gonzalez M and Audit E, Journal of Applied Physics. Vol. 107, pp. 083302/19  (2010). 
Abstract: We have studied the dynamics of strong radiative shocks generated with the highenergy subnanosecond iodine laser at Prague Asterix Laser System facility (Prague) over long time scales, up to 100 ns. These shock waves are characterized by a developed radiative precursor, a radiation driven ionization wave in front of the density jump of the shock. Electronic density profiles are measured at different times after the laser pulse and at different distances from the axis of the shock tube. A new feature, described as a split precursor, has been observed. Comparisons with twodimensional computations are shown. 
BibTeX:
@article{Busquet2010, author = {Busquet, M. and Thais, F. and Gonzalez, M. and Audit, E.}, title = {Measure of precursor electron density profiles of laser launched radiative shocks}, journal = {Journal of Applied Physics}, year = {2010}, volume = {107}, pages = {083302/19}, url = {http://dx.doi.org/10.1063/1.3330636}, doi = {10.1063/1.3330636} } 
"Xray crystal spectrometer for opacities measurements in the 818 Å spectral range at the LULI laser facility" Reverdin C, Thais F, Loisel G and Bougeard M, Review of Scientific Instruments. Vol. 81, pp. 10E327_15 (2010). 
Abstract: An xray crystal spectrometer was built in order to measure opacities in the 8â€“18 Ä¹ spectral range with an average spectral resolution of (λ/δλ)  400. It has been successfully used at the LULI2000 laser facility ( See C. Sauteret, rapport LULI 2001, 88 (2002) at école Polytechnique (France) to measure in the same experimental conditions the 2p3d transitions of several elements with the neighboring atomic number Z: Fe, Ni, Cu, and Ge [ G. Loisel et al., High Energy Density Phys. 5, 173 (2009) ]. Hence, a spectrometer with a wide spectral range is needed. This spectrometer features two lines of sight. In this example, one line of sight looks through the sample and the other one is looking directly at the backlighter emission. Both are outfitted with a spherical condensing mirror. A TlAP crystal is used for spectral dispersion. Detection is made with an image plate Fuji BAS TR2025, which is sensitive to x rays. We present some experimental results showing the performances of this spectrometer. 
BibTeX:
@article{Reverdin2010, author = {Reverdin, C. and Thais, F. and Loisel, G. and Bougeard, M.}, title = {Xray crystal spectrometer for opacities measurements in the 818 Ä¹ spectral range at the LULI laser facility}, journal = {Review of Scientific Instruments}, year = {2010}, volume = {81}, pages = {10E327_15}, url = {http://link.aip.org/link/?RSI/81/10E327}, doi = {10.1063/1.3491285} } 
2009 
"MultiCode Ab Initio Calculation of Ionization Distributions and Radiation Losses for Tungsten in Tokamak Plasmas" Ralchenko Yu, J. Abdallah JR, BarShalom A, Bauche J, BaucheArnoult C, Bowen C, Chung HK, Colgan J, Faussurier G, Fontes CJ, Foster M, de Gaufridy de Dortan F, Golovkin I, Hansen SB, Lee RW, Novikov V, Oreg J, Peyrusse O, Poirier M, Sasaki A, Scott H et Zhang HL, AIP Conference Proceedings. Vol. 1161(1), pp. 242250, (2009). 
Abstract: We present calculations of ionization balance and radiative power losses for tungsten in magnetic fusion plasmas. The simulations were performed within the framework of NonLocal Thermodynamic Equilibrium (NLTE) Code Comparison Workshops utilizing several independent collisionalradiative models. The calculations generally agree with each other; however, a clear disagreement with experimental ionization distributions at low temperatures 2 keV<T_{e}<3 keV is observed. Comparison is made with other calculations. The obtained results can be used in planning new experiments in magnetic confinement fusion. 
BibTeX:
@article{Ralchenko2009, author = {Yu. Ralchenko and J. Abdallah Jr. and A. BarShalom and J. Bauche and C. BaucheArnoult and C. Bowen and H.?K. Chung and J. Colgan and G. Faussurier and C. J. Fontes and M. Foster and F. de Gaufridy de Dortan and I. Golovkin and S. B. Hansen and R. W. Lee and V. Novikov and J. Oreg and O. Peyrusse and M. Poirier and A. Sasaki and H. Scott and H. L. Zhang}, title = {MultiCode Ab Initio Calculation of Ionization Distributions and Radiation Losses for Tungsten in Tokamak Plasmas}, journal = {AIP Conference Proceedings}, year = {2009}, volume = {1161}, number = {1}, pages = {242250}, url = {https://aip.scitation.org/doi/abs/10.1063/1.3241195}, doi = {10.1063/1.3241195} } 
"Excitonexciton interactions in CdWO4 irradiated by intense femtosecond vacuum ultraviolet pulses" Kirm M, Nagirnyi V, Feldbach E, De Grazia M, Carré B, Merdji H, Guizard S, Geoffroy G, Gaudin J, Fedorov N, Martin P, Vasil'ev A and Belsky A, Physical Review  B: Solid State (former title). Vol. 79, pp. 233103\_14  (2009). 
Abstract: Excitonexciton interaction is experimentally revealed and quantitatively analyzed in a wide bandgap scintillator material CdWO4. Under highintensity femtosecond vacuum ultraviolet excitation, the CdWO4 luminescence is quenched, while its decay becomes essentially nonexponential. We propose an analytical model,which successfully reproduces the decay kinetics recorded in a wide range of excitation densities. The dipoledipole interaction between excitons leading to their nonradiative decay is shown to be the main cause of a nonproportional response common for many scintillators. 
BibTeX:
@article{Kirm2009, author = {Kirm, M. and Nagirnyi, V. and Feldbach, E. and De Grazia, M. and Carré, B. and Merdji, H. and Guizard, S. and Geoffroy, G. and Gaudin, J. and Fedorov, N. and Martin, P. and Vasil'ev, A. and Belsky, A.}, title = {Excitonexciton interactions in CdWO4 irradiated by intense femtosecond vacuum ultraviolet pulses}, journal = {Physical Review  B: Solid State (former title)}, year = {2009}, volume = {79}, pages = {23310314}, url = {http://prb.aps.org/abstract/PRB/v79/i23/e233103}, doi = {10.1103/PhysRevB.79.233103} } 
"Absorption spectroscopy of mid and neighboring Z plasmas: iron, nickel, copper and germanium" Loisel G, Arnault P, BastianiCeccotti S, Blenski T, Caillaud T, Fariaut J, Folsner W, Gilleron F, Pain JC, Poirier M, Reverdin C, Silvert V, Thais F, TurckChièze S and Villette B, High Energy Density Physics. Vol. 5, pp. 173181  (2009). 
Abstract: Opacities of four medium Z element plasmas (iron, nickel, copper and germanium) have been measured at the LULI2000 facility in similar conditions: temperatures between 15 and 25 eV and densities between 2 and 10 mg/cm3, in a wavelength range (8â€“18 Ä¹) including the strong 2pâ€“3d structures. Two laser beams from the LULI facility were used in the nanosecondpicosecond configuration. The NANO2000 beam (at λ = 0.53 Âµm) heated a gold hohlraum with an energy between 30 and 150 J with a duration of 0.6 ns. Samples covering half a hohlraum hole were thus radiatively heated. The picosecond pulse PICO2000 beam (at λ = 1.053 Âµm) has been used to produce a short (about 10 ps) Xray backlighter in order to reduce time variations of temperatures and densities during the measurement. A crystal highresolution spectrometer was used as the main diagnostic to record at the same time the nonabsorbed and the absorbed backlighter spectra. Radiation temperatures were measured using a broadband spectrometer. 1D and 2D simulations have been performed in order to estimate hydrodynamic plasmas parameters. The measured spectra have been compared with theoretical ones obtained using either the superconfiguration code SCO or the detailed term accounting code HULLAC. These comparisons allow us to check the modeling of the statistical broadening and of the spinorbit splitting of the 2pâ€“3d transitions and related effects such as the interaction between relativistic subconfigurations belonging to the same nonrelativistic configuration. 
BibTeX:
@article{Loisel2009, author = {Loisel, G. and Arnault, P. and BastianiCeccotti, S. and Blenski, T.J. and Caillaud, T. and Fariaut, J. and Folsner, W. and Gilleron, F. and Pain, J.C. and Poirier, M. and Reverdin, C. and Silvert, V. and Thais, F. and TurckChièze, S. and Villette, B.}, title = {Absorption spectroscopy of mid and neighboring Z plasmas: iron, nickel, copper and germanium}, journal = {High Energy Density Physics}, year = {2009}, volume = {5}, pages = {173181}, url = {http://dx.doi.org/10.1016/j.hedp.2009.05.015}, doi = {10.1016/j.hedp.2009.05.015} } 
"Variational AverageAtom in Quantum Plasmas (VAAQP) A check of thermodynamic consistency" Piron R, Blenski T and Cichocki B, High Energy Density Physics. Vol. 5, pp. 258262  (2009). 
Abstract: A new code called VAAQP (Variational AverageAtom in Quantum Plasmas) is presented. The conceptual model on which the code is based, as well as the important results of previous studies are briefly discussed. The code is based on a new fully variational model of equilibrium dense plasmas employing a quantal treatment of all electrons. VAAQP can calculate the AverageAtom structure and the mean ionization from the variational equations satisfying the virial theorem and without imposing the neutrality of the WignerSeitz sphere. The formula obtained for the electron pressure is simple and does not require any numerical differentiation. A description of the principal features of the code is given. The thermodynamic consistency of the results obtained with VAAQP is shown by a comparison with another approach for the aluminium 2 eV isotherm. An initial comparison to an Infernotype model is also presented. 
BibTeX:
@article{Piron2009, author = {Piron, R. and Blenski, T.J. and Cichocki, B.}, title = {Variational AverageAtom in Quantum Plasmas (VAAQP) A check of thermodynamic consistency}, journal = {High Energy Density Physics}, year = {2009}, volume = {5}, pages = {258262}, url = {http://dx.doi.org/10.1016/j.hedp.2009.05.013}, doi = {10.1016/j.hedp.2009.05.013} } 
"Variational AverageAtom in Quantum Plasmas(VAAQP)  first numerical results." Piron R, Blenski T and Cichocki B, Journal of Physics AMathematical and Theoretical. Vol. 42, pp. 214059  (2009). 
Abstract: The work on a new fully variational model of averageatom inquantum plasmas using a numerical code called VAAQP is reported. A briefdescription of the code is given. Application to aluminium at solid densityand temperatures between 0.05 and 12 eV is presented. Comparisons to resultsobtained using other approaches are also shown and discussed. The results provethe feasibility of the variational model in the warm dense matter regime. Effectsof the variational treatment can lead in this region to significant differences withrespect to existing models. 
BibTeX:
@article{Piron2009a, author = {Piron, R. and Blenski, T.J. and Cichocki, B.}, title = {Variational AverageAtom in Quantum Plasmas(VAAQP)  first numerical results.}, journal = {Journal of Physics AMathematical and Theoretical}, year = {2009}, volume = {42}, pages = {214059}, url = {http://dx.doi.org/10.1088/17518113/42/21/214059}, doi = {10.1088/17518113/42/21/214059} } 
"Highly efficient sparsematrix inversion techniques and average procedures applied to collisionalradiative codes" Poirier M and de Gaufridy de Dortan F, High Energy Density Physics. Vol. 5, pp. 328336  (2009). 
Abstract: The behavior of nonlocal thermalequilibrium (NLTE) plasmas plays a central role in many fields of modernday physics, such as laserproduced plasmas, astrophysics, inertial or magnetic confinement fusion devices, and Xray sources. In steadystate cases the proper description of these plasmas may require the solution of thousands of linear rate equations. A possible simplification for this numerical task lies in some form of statistical averaging, such as the averaging over configurations or superconfigurations. However, to assess the validity of such an averaging procedure and to handle cases where isolated lines play an important role, it will be important to treat detailed levels systems. This involves matrices with potentially billions of elements, which are rather sparse but still involve thousands of diagonals above and below the main one. We propose here a numerical algorithm based on the LU decomposition for such linear systems. It will be shown that this method is ordersofmagnitude faster than the traditional Gauss elimination. Moreover, it is found that there are no convergence or accuracy issues, which are found when using methods based on conjugate gradients or minimization. Among cases treated at the last NLTEkineticscode meeting, krypton and tungsten plasmas are considered. Furthermore, to assess the validity of configuration averaging, several criteria are discussed. While a criterion based on detailed balance is relevant in cases not too far from LTE, it is found to be insufficient in general. An alternate criterion based on the inspection of the influence of an arbitrary configuration temperature is proposed and tested successfully. 
BibTeX:
@article{Poirier2009, author = {Poirier, M. and de Gaufridy de Dortan, F.}, title = {Highly efficient sparsematrix inversion techniques and average procedures applied to collisionalradiative codes}, journal = {High Energy Density Physics}, year = {2009}, volume = {5}, pages = {328336}, url = {http://dx.doi.org/10.1016/j.hedp.2009.03.012}, doi = {10.1016/j.hedp.2009.03.012} } 
"On plasma radiative properties in stellar conditions" TurckChieze S, Delahaye F, Gilles D, Loisel G and Piau L, High Energy Density Physics. Vol. 5, pp. 132138  (2009). 
Abstract: The knowledge of stellar evolution is evolving quickly thanks to an increased number of opportunities to scrutinize the stellar internal plasma properties by stellar seismology and by 1D and 3D simulations. These new tools help us to introduce the internal dynamical phenomena in stellar modeling. A proper inclusion of these processes supposes a real confidence in the microscopic physics used, partly checked by solar or stellar acoustic modes. In the present paper we first recall which fundamental physics has been recently verified by helioseismology. Then we recall that opacity is an important ingredient of the secular evolution of stars and we point out why it is necessary to measure absorption coefficients and degrees of ionization in the laboratory for some well identified astrophysical conditions. We examine two specific experimental conditions which are accessible to large laser facilities and are suitable to solve some interesting questions of the stellar community: are the solar internal radiative interactions properly estimated and what is the proper role of the opacity in the excitation of the nonradial modes in the envelop of the ÃŸ Cepheids and the Be stars? At the end of the paper we point out the difficulties of the experimental approach that we need to overcome. 
BibTeX:
@article{TurckChieze2009, author = {TurckChieze, S. and Delahaye, F. and Gilles, D. and Loisel, G. and Piau, L.}, title = {On plasma radiative properties in stellar conditions}, journal = {High Energy Density Physics}, year = {2009}, volume = {5}, pages = {132138}, url = {http://dx.doi.org/10.1016/j.hedp.2009.06.007}, doi = {10.1016/j.hedp.2009.06.007} } 
"Atome moyen variationnel dans les plasmas quantiques" Piron R, In Physique.. Thesis at: Ecole Polytechnique.  (2009). 
Abstract: Le calcul des propriétés radiatives des plasmas denses fait en général appel au concept d'atome dans un plasma. Parmi les modèles qui définissent un tel concept, les modèles d'atome moyen représentent souvent un point de départ indispensable avant des approches statistiques plus sophistiquées. En outre, ils permettent de calculer les propriétés thermodynamiques ainsi que certains coefficients de transport. Depuis l'application du modèle quasiclassique de ThomasFermi aux plasmas denses par Feynman, Metropolis et Teller, toutes ses généralisations quantiques ont conduit à des modèles qui présentent des inconsistances thermodynamiques. Ce travail porte sur un modèle variationnel d'atome moyen pour la description des plasmas denses. Contrairement aux autres modèles, ce dernier donne, par construction, accès à l'équilibre thermodynamique et vérifie le théorème du viriel. Afin de résoudre les équations de ce modèle, un code nommé VAAQP (Variational AverageAtom in Quantum Plasmas) a été réalisé. Il permet notamment le calcul de l'équation d'état des plasmas denses. Après un état de l'art des modèles d'atome moyen, le formalisme du modèle variationnel est décrit dans ses versions ThomasFermi, quantique nonrelativiste et quantique relativiste. La validité du théorème du viriel pour ce modèle est démontrée et l'inconsistance thermodynamique des autres modèles est expliquée. Les méthodes numériques qui sont appliquées dans VAAQP sont ensuite exposées. Enfin, les résultats obtenus avec le modèle variationnel, concernant les équations d'état, sont commentés et comparés aux résultats d'autres modèles, dont le modèle INFERNO, ainsi qu'à des résultats d'expériences sur les adiabatiques d'Hugoniot. 
BibTeX:
@phdthesis{PhdThesisPiron2009, author = {Piron, R.}, title = {Atome moyen variationnel dans les plasmas quantiques}, booktitle = {Physique}, school = {Ecole Polytechnique}, year = {2009}, url = {http://tel.archivesouvertes.fr/tel00446558/fr/} } 
"FEMTOSECOND LASER ABLATION OF DIELECTRICS: EXPERIMENTAL STUDIES OF FUNDAMENTAL PROCESSES." Guizard S, Fedorov N, Geoffroy G, Belsky A, Martin P, Bachau H and Vasil'ev A, In 10th International Conference on Laser Ablation (COLA  2009). Singapour  (2009). 
Abstract: In the field of laser ablation of wide band gap materials by ultrashort laser pulses, there has been a long debate regarding the excitation and energy deposition mechanism. This is due to the lack of direct experimental investigations, which have been mostly limited to the measurement of ablation threshold. In principle the energy balance of the interaction is completely characterised if one measure the excited carrier's density and their energy distribution. We have used an original time resolved pumpprobe interferometry technique [1] to measure in real time the excited carrier density in the solid, at intensities below and above ablation threshold. The evolution of the carrier density as a function of incident intensity for different pulse duration in the range 50fs to 1.2ps suggests that multiphoton ionization is the dominant excitation mechanism. This conclusion is valid for all the materials investigated, namely SiO2 Al2O3 and MgO [2]. This results have been recently been confirmed [3]. Furthermore, we will present unpublished data of recent experiments performed with longer pulse durations (up to 10ps) and also with double pulse excitation, which bring new information on the excitation and propagation mechanisms. To measure the energy distribution of the photoexcited carriers, we used photoelectron spectroscopy. After excitation with a single pulse (TiSa laser, 50fs pulse duration), the kinetic energy spectra of electron emitted at the surface of a quartz sample (αSiO2) is measured as a function of laser intensity. We have shown that energies up to 30 eV, i.e. more than 20 times the incident the photon energy, can be observed, at intensities of the order of 1013W/cm2, i.e. far below breakdown threshold [4]. To interpret this observation, we have developed a new model, describing the heating of carriers in the conduction band as a succession of multiphoton transition enhanced by resonance with different branches of the conduction band. This mechanism is extremely efficient, at lest 100 times more efficient than in atoms, and should be taken into account in the modeling of laser induced breakdown. Finally, we have observed, with a new MEB providing images with resolution better than 10nm on dielectrics, the surface of craters after ablation under various experimental conditions (number of shots, polarization, wavelength, etc). Unexpectedly, the structures observed very much depends upon the material considered (SiO2, Al2O3, MgO, KDP) showing that ablation is not only a pure plasma process, but that the materials properties play a major role in the final result of ablation. [1] Audebert P., Daguzan Ph., Guizard S., et al. Physical Review Letters 52, p. 1994.[2] Quéré F, Guizard S, Martin P, Europhys. Lett. 56, p. 138144, 2001. [3] V.V. Temnov, et al., Phys. Rev. Lett. 97, p. 237403, 2006. [4] Belsky A, Martin P, Bachau H, Guizard S. et al.EuroPhysics Letters 67 (2): p.301, 2004. 
BibTeX:
@inproceedings{InproGuizard2009, author = {Guizard, S. and Fedorov, N. and Geoffroy, G. and Belsky, A. and Martin, P. and Bachau, H. and Vasil'ev, A.}, title = {FEMTOSECOND LASER ABLATION OF DIELECTRICS: EXPERIMENTAL STUDIES OF FUNDAMENTAL PROCESSES.}, booktitle = {10th International Conference on Laser Ablation (COLA  2009)}, year = {2009} } 
2008 
"Les supraconfigurations : un outil pour l'étude des plasmas d'ions multichargés à l'ETL" Blenski T and Pain JC, Chocs. Vol. 36, pp. 1321  (2008). 
Abstract: Afin de modéliser l'absorption et l'émission du rayonnement par les plasmas, il s'avère nécessaire de prendre en compte un très grand nombre de configurations électroniques des ions et de décrire de manière réaliste leurs structures. La méthode des supraconfigurationsa été introduite afin de calculer l'opacité des plasmas à l'équilibre thermodynamique local.Elle constitue une approche statistique de la physique atomique des plasmas denses audelàdu modèle de l'Atome Moyen. Chaque espèce ionique est décrite par un ensemble de supraconfigurations, chaque supraconfiguration représentant un groupe de configurations électroniques. Dans cet article, nous présentons les principes de la méthode des supraconfigurations ainsi que sa réalisation pratique dans un code de calcul d'opacité (SCO). Une des spécificités de ce code est l'inclusion de l'écrantage statique des ions par le plasma. Ce modèle a été confronté aux résultats d'une série d'expériences de mesure d'opacité dans lesquelles la densité du plasma était de l'ordre de 0.01 g/cm3. En principe, ce modèle permettra également l'étude des effets de densité (notamment de l'ionisation par pression) sur l'opacité et sur l'équation d'état des plasmas plus denses.AbstractIn order to model absorption and emission of radiation by plasmas it is necessary toaccount for a huge number of ion configurations and to use a realistic description of theirelectronic structures. The superconfiguration method has been introduced in order to calculateopacities in plasmas at local thermodynamic equilibrium. This method is a statisticalapproach to ions allowing one to study atomic physics of dense plasmas beyond the AverageAtom model. Each ionic species is described by a group of superconfigurations and each superconfiguration represents in turn a certain number of configurations. In this article we present the basic principles of the superconfiguration method as well as its practicalimplementation in a numerical code (SCO). One of the main features of that code is the inclusion of static screening of ions by plasma. Results of this model have been compared to results of published opacity measurements in which plasma density was of the order of 0.01 g/cm3. In principle the model will allow us to study plasma density effects (for example pressure ionization) on opacity and equation of state in case of higher density plasmas. 
BibTeX:
@article{Blenski2008, author = {Blenski, T. and Pain, J.C.}, title = {Les supraconfigurations : un outil pour l'étude des plasmas d'ions multichargés à l'ETL}, journal = {Chocs}, year = {2008}, volume = {36}, pages = {1321} } 
"On various validity criteria for the configuration average in collisionalradiative codes" Poirier M, Journal of Physics B. Atomic, Molecular and Optical Physics. Vol. 41, pp. 025701  (2008). 
Abstract: The characterization of outoflocalthermalequilibrium plasmas requires the use of collisionalradiative kinetic equations. This leads to the solution of large linear systems, for which statistical treatments such as configuration average may bring considerable simplification. In order to check the validity of this procedure, a criterion based on the comparison between a partialrate systems and the SahaBoltzmann solution is discussed in detail here. Several forms of this criterion are discussed. The interest of these variants is that they involve each type of relevant transition (collisional or radiative), which allows one to check separately the influence of each of these processes on the configurationaverage validity. The method is illustrated by a chargedistribution analysis in carbon and neon plasmas. Finally, it is demonstrated that when the energy dispersion of every populated configuration is smaller than the electron thermal energy, the proposed criterion is fulfilled in each of its forms. 
BibTeX:
@article{Poirier2008, author = {Poirier, M.}, title = {On various validity criteria for the configuration average in collisionalradiative codes}, journal = {Journal of Physics B. Atomic, Molecular and Optical Physics}, year = {2008}, volume = {41}, pages = {025701}, url = {http://dx.doi.org/10.1088/09534075/41/2/025701}, doi = {10.1088/09534075/41/2/025701} } 
"Relaxation of electronic excitations in widegap crystals studied by femtosecond interferometry technique" Nagirnyi V, Geoffroy G, Guizard S, Kirm M and Kotlov A, Physics of the Solid State. Vol. 50(9), pp. 17841788  (2008). 
Abstract: Timeresolved interferometry with a 100fs temporal resolution was applied for the first time to studying the relaxation of electronic excitations in complex oxides, namely, tungstates CDWO_{4} with a crystal lattice of the wolframitetype and CaWO_{4} with a scheelitetype lattice. Two stages of charge carrier relaxation, namely, very fast carrier trapping in 200 fs resulting in selftrapped exciton formation and a relatively slow picosecond relaxation process probably due to configurational relaxation within the oxyanion molecule and modification of the surrounding lattice, are revealed in tungstate crystals. Corresponding models of selftrapped exciton creation in tungstate crystals are discussed. 
BibTeX:
@article{Nagirnyi2008, author = {Nagirnyi, V. and Geoffroy, G. and Guizard, S. and Kirm, M. and Kotlov, A.}, title = {Relaxation of electronic excitations in widegap crystals studied by femtosecond interferometry technique}, journal = {Physics of the Solid State}, year = {2008}, volume = {50}, number = {9}, pages = {17841788}, url = {http://link.springer.com/article/10.1134%2FS1063783408090382}, doi = {10.1134/S1063783408090382} } 
2007 
"Interpretation of some Xray and XUV absorption experiments using SCO" Arnault P, Blenski T and Dejonghe G, High Energy Density Physics. Vol. 3, pp. 17  (2007). 
Abstract: We review some Xray and XUV absorption experiments on aluminium and germanium making systematic comparison between theory and experiment with the help of the superconfiguration code SCO. The objective is to identify areas that require further theoretical development. As for the low and medium Z elements considered, the statistical term treatment essential in the superconfiguration method is less physically sound than a detailed linebyline treatment. Nevertheless, we comment on recent spectroscopic measurements at near solid density that suggest a larger domain of validity for statistical approximation than previously thought. We will also address some specific theoretical issues that affect the absorption structures such as orbital relaxation in the final state of optical transitions and the broadening of spectral lines by collisions with electrons. 
BibTeX:
@article{Arnault2007, author = {Arnault, P. and Blenski, T.J. and Dejonghe, G.}, title = {Interpretation of some Xray and XUV absorption experiments using SCO}, journal = {High Energy Density Physics}, year = {2007}, volume = {3}, pages = {17}, url = {http://dx.doi.org/10.1016/j.hedp.2007.01.001}, doi = {10.1016/j.hedp.2007.01.001} } 
"Analysis of the Xray and timeresolved XUV emission of laser produced Xe and Kr plasmas" BastianiCeccotti S, Kontogiannopoulos N, Marquès JR, Tzortzakis S, Lecherbourg L, Thais F, Matsushima I, Peyrusse O and ChenaisPopovics C, High Energy Density Physics. Vol. 3, pp. 2027  (2007). 
Abstract: A frequencydoubled laser beam of the Nd:glass kilojoule nanosecond LULI2000 facility (1.5 ns duration, 200â€“400 J energy, 0.53 Âµm wavelength) was focused on a Xe or Kr gas jet. The plasma was simultaneously diagnosed with Xray (in the wavelength range of 6â€“8 Ä¹ for Kr and of 12â€“15 Ä¹ for Xe) and timeresolved XUV (20â€“200 Ä¹) emission spectroscopy. Electron density and temperature as well as the ionization charge were measured by timeresolved Thomson scattering of the heating laser pulse. The spectra are compared with the calculations performed with the NLTE collisionalradiative code AVERROES/TRANSPEC. Best fits of the Xray and XUV spectra obtained are presented. The measured charge distribution and dynamics is analyzed using the simultaneous Thomson scattering diagnostic. 
BibTeX:
@article{BastianiCeccotti2007, author = {BastianiCeccotti, S. and Kontogiannopoulos, N. and Marquès, J.R. and Tzortzakis, S. and Lecherbourg, L. and Thais, F. and Matsushima, I. and Peyrusse, O. and ChenaisPopovics, C.}, title = {Analysis of the Xray and timeresolved XUV emission of laser produced Xe and Kr plasmas}, journal = {High Energy Density Physics}, year = {2007}, volume = {3}, pages = {2027}, url = {http://dx.doi.org/10.1016/j.hedp.2007.01.004}, doi = {10.1016/j.hedp.2007.01.004} } 
"Variational theory of AverageAtom and superconfigurations in quantum plasmas" Blenski T and Cichocki B, Physical Review E. Vol. 75, pp. 056402  (2007). 
Abstract: Models of screened ions in equilibrium plasmas with all quantum electrons are important in opacity and equation of state calculations. Although such models have to be derived from variational principles, up to now existing models have not been fully variational. In this paper a fully variational theory respecting virial theorem is proposed  all variables are variational except the parameters defining the equilibrium, i.e., the temperature T, the ion density ni and the atomic number Z. The theory is applied to the quasiclassical ThomasFermi (TF) atom, the quantum average atom (QAA), and the superconfigurations (SC) in plasmas. Both the selfconsistentfield (SCF) equations for the electronic structure and the condition for the mean ionization Z* are found from minimization of a thermodynamic potential. This potential is constructed using the cluster expansion of the plasma free energy from which the zero and the firstorder terms are retained. In the zero order the free energy per ion is that of the quantum homogeneous plasma of an unknown freeelectron density n0=Z*ni occupying the volume 1/ni. In the first order, ions submerged in this plasma are considered and local neutrality is assumed. These ions are considered in the infinite space without imposing the neutrality of the WignerSeitz (WS) cell. As in the Inferno model, a central cavity of a radius R is introduced, however, the value of R is unknown a priori. The charge density due to noncentral ions is zero inside the cavity and equals en0 outside. The firstorder contribution to free energy per ion is the difference between the free energy of the system central ion + infinite plasma and the free energy of the system infinite plasma. An important part of the approach is an ionization model (IM), which is a relation between the mean ionization charge Z* and the firstorder structure variables. Both the IM and the local neutrality are respected in the minimization procedure. The correct IM in the TF case is found to be Z−Z*= Integral d3r [n(vec(r))−n0], where n(vec(r)) is the firstorder electron density. It is shown that in the QAA case the same IM has to be used and that other IMs lead to unphysical solutions. With this IM R becomes in both cases (TF and QAA) equal to the WS radius and the variational calculation leads to SCF equations in an infinite plasma while n0 (or equivalently Z*) is to be found from the condition Integral d3r Theta(r−R) Vel(vec(r))=0, where Theta denotes Heaviside function and Vel(vec(r)) is the SCF electrostatic potential. In the SC case results are similar except that averages over all superconfigurations appear. In the TF case the condition for n0 gives the neutrality of the WS sphere and one gets the classical TF ionincell average atom. The situation is different in the QAA and in the SC cases in which the cavity is not neutral and the SCF potential Vel(vec(r)) is not zero outside the cavity. Due to the fully variational character of our approach the expression for the thermodynamic pressure in all cases does not require any numerical differentiation and is consistent with the virial theorem. 
BibTeX:
@article{Blenski2007, author = {Blenski, T.J. and Cichocki, B.}, title = {Variational theory of AverageAtom and superconfigurations in quantum plasmas}, journal = {Physical Review E}, year = {2007}, volume = {75}, pages = {056402}, url = {http://dx.doi.org/10.1103/PhysRevE.75.056402} } 
"Variational approach to the AverageAtominjellium and superconfigurationsinjellium models with all electrons treated quantummechanically" Blenski T and Cichocki B, High Energy Density Physics. Vol. 3, pp. 3447  (2007). 
Abstract: Models of average atom and superconfigurations in plasmas with full quantum description of all electrons are important in opacity and EOS calculations, especially in case of high density plasmas in which pressure ionization phenomena can occur. However variational formulation of models becomes difficult when quantum free electrons are considered.In our approach we use a cluster expansion of the free energy expression from which we retain the sum of the zero and of the first order terms. In the zero order the free energy is that of the homogeneous jellium of an unknown free electron density. In the first order we consider a one selfconsistentfield (SCF) average atoms or ions submerged in this jellium. The SCF potential is assumed to be localized. We consider the firstorder atoms or ion in the whole space without imposing the neutrality of the WignerSeitz cell. The important part of the model is a relation between the average ion charge and the localized part of electron density that is called ionizationmodel.The minimization procedure of the free energy is performed with respect to all variables except these characterizing the plasma equilibrium i.e. except the temperature, the ion density and the atomic number. It is interesting that when the electron density is taken in the ThomasFermi (TF) approximation together with a specific choice of the ionization model, our approach correctly leads to the classical TF ionincell average atom. It also appears that the same ionization model has to be used in the quantum case and that other ionization models lead to unphysical solutions. This observation is important with respect to the choice of correct ionization model in the case of superconfigurations in jellium.Due to the fully variational character of our approach the resulting expression for the thermodynamic pressure in all considered cases is simple and does not require any numerical differentiation. 
BibTeX:
@article{Blenski2007a, author = {Blenski, T.J. and Cichocki, B.}, title = {Variational approach to the AverageAtominjellium and superconfigurationsinjellium models with all electrons treated quantummechanically}, journal = {High Energy Density Physics}, year = {2007}, volume = {3}, pages = {3447}, url = {http://dx.doi.org/10.1016/j.hedp.2007.01.006} } 
"Effect of lateral radiative losses on radiative shock propagation" Busquet M, Audit E, Gonzalez M, Stehle C, Thais F, Acef O, Bauduin D, Barroso P, Rus B, Kozlova M, Polan J and Mocek T, High Energy Density Physics. Vol. 3, pp. 811  (2007). 
Abstract: Experimental and numerical studies of radiative shocks, of interest as scaled astrophysical objects, have been performed. Experiments were conducted at the PALS facility in Prague with a xenon filled minishock tube using a laser accelerated plastic pusher. Numerical simulations of the hydrodynamics including radiation effects have been performed with the 3D code HERACLES. Measurements have been made of the electronic density of the shocked gas and of the time history of the position of the radiative precursor. Simulations and experimental results show good agreement when lateral radiative losses are taken into account, including a wall albedo of 40%. 
BibTeX:
@article{Busquet2007, author = {Busquet, M. and Audit, E. and Gonzalez, M. and Stehle, C. and Thais, F. and Acef, O. and Bauduin, D. and Barroso, P. and Rus, B. and Kozlova, M. and Polan, J. and Mocek, T.}, title = {Effect of lateral radiative losses on radiative shock propagation}, journal = {High Energy Density Physics}, year = {2007}, volume = {3}, pages = {811}, url = {http://dx.doi.org/10.1016/j.hedp.2007.01.002}, doi = {10.1016/j.hedp.2007.01.002} } 
"Highgain directdrive inertial confinement fusion for the Laser Mégajoule: recent progress" Canaud B, Garaude F, Ballereau P, Bourgade J, Clique C, Dureau D, Houry M, Jaouen S, Jourdren H, Lecler N, Masse L, Masson A, Quach R, Piron R, Riz D, Van der Vliet J, Temporal M, Delettrez J and McKenty P, Plasma Physics and Controlled Fusion. Vol. 49, pp. B601B610  (2007). 
Abstract: Recent progress in highgain directdrive inertial confinement fusion with the laser Mégajoule is reviewed. A new baseline directdrive target design is presented which implodes with a twocones irradiation pattern of indirectdrive beam configuration and zooming. Perturbation amplitudes and correlated growth rates of hydrodynamic instabilities in the compressed core of a directly driven inertial confinement fusion capsule are analyzed in planar and spherical geometries, with and without heat conduction, in the unsteady state regime of the deceleration. Shock propagation in heterogeneous media is addressed in the context of first shock. The neutron and photon emissions of highgain directdrive target are characterized. Numerical interpretations of directly driven homothetic cryogenic D2 target implosion experiments on the Omega facility are presented. 
BibTeX:
@article{Canaud2007, author = {Canaud, B. and Garaude, F. and Ballereau, P. and Bourgade, J.L. and Clique, C. and Dureau, D. and Houry, M. and Jaouen, S. and Jourdren, H. and Lecler, N. and Masse, L. and Masson, A. and Quach, R. and Piron, R. and Riz, D. and Van der Vliet, J. and Temporal, M. and Delettrez, J.A. and McKenty, P.W.}, title = {Highgain directdrive inertial confinement fusion for the Laser Mégajoule: recent progress}, journal = {Plasma Physics and Controlled Fusion}, year = {2007}, volume = {49}, pages = {B601B610}, url = {http://dx.doi.org/10.1088/07413335/49/12B/S56}, doi = {10.1088/07413335/49/12B/S56} } 
"Measurement of XUVabsorption spectra of ZnS radiatively heated foils" Kontogiannopoulos N, BastianiCeccotti S, Thais F, ChenaisPopovics C, Sauvan P, Schott R, Folsner W, Arnault P, Poirier M and Blenski T, High Energy Density Physics. Vol. 3, pp. 149155  (2007). 
Abstract: Timeresolved absorption of zinc sulfide (ZnS) and aluminum in the XUVrange has been measured. Thin foils in conditions close to local thermodynamic equilibrium were heated by radiation from laserirradiated gold spherical cavities. Analysis of the aluminum foil radiative hydrodynamic expansion, based on the detailed atomic calculations of its absorption spectra, showed that the cavity emitted flux that heated the absorption foils corresponds to a radiation temperature in the range 55 60 eV. Comparison of the ZnS absorption spectra with calculations based on a superconfiguration approach identified the presence of species Zn6+  Zn8+ and S5+  S6+. Based on the validation of the radiative source simulations, experimental spectra were then compared to calculations performed by postprocessing the radiative hydrodynamic simulations of ZnS. Satisfying agreement is found when temperature gradients are accounted for. 
BibTeX:
@article{Kontogiannopoulos2007, author = {Kontogiannopoulos, N. and BastianiCeccotti, S. and Thais, F. and ChenaisPopovics, C. and Sauvan, P. and Schott, R. and Folsner, W. and Arnault, P. and Poirier, M. and Blenski, T.J.}, title = {Measurement of XUVabsorption spectra of ZnS radiatively heated foils}, journal = {High Energy Density Physics}, year = {2007}, volume = {3}, pages = {149155}, url = {http://dx.doi.org/10.1016/j.hedp.2007.02.011}, doi = {10.1016/j.hedp.2007.02.011} } 
"A comparison between detailed and configurationaveraged collisional radiative codes applied to nonlocalthermalequilibrium plasmas" Poirier M and de Gaufridy de Dortan F, Journal of Applied Physics. Vol. 101, pp. 063308  (2007). 
Abstract: A collisionalradiative model describing nonlocalthermodynamicequilibrium plasmas is developed. It is based on the HULLAC (Hebrew University Lawrence Livermore Atomic Code) suite for the transitions rates, in the zerotemperature radiation field hypothesis. Two variants of the model are presented: the first one is configuration averaged, while the second one is a detailed level version. Comparisons are made between them in the case of a carbon plasma; they show that the configurationaveraged code gives correct results for an electronic temperature T_{e} = 10eV (or higher) but fails at lower temperatures such as T_{e} = 1eV. The validity of the configurationaveraged approximation is discussed: the intuitive criterion requiring that the average configurationenergy dispersion must be less than the electron thermal energy turns out to be a necessary but far from sufficient condition. Another condition based on the resolution of a modified rateequation system is proposed. Its efficiency is emphasized in the case of lowtemperature plasmas. Finally, it is shown that nearthreshold autoionization cascade processes may induce a severe failure of the configurationaverage formalism. 
BibTeX:
@article{Poirier2007, author = {Poirier, M. and de Gaufridy de Dortan, F.}, title = {A comparison between detailed and configurationaveraged collisional radiative codes applied to nonlocalthermalequilibrium plasmas}, journal = {Journal of Applied Physics}, year = {2007}, volume = {101}, pages = {063308}, url = {http://dx.doi.org/10.1063/1.2713085}, doi = {10.1063/1.2713085} } 
"Revisiting nonlocal electronenergy transport in inertialfusion conditions" Schurtz G, Gary S, Hulin S, ChenaisPopovics C, Gauthier J, Thais F, Breil J, Durut J, Feugeas J, Maire P, Nicolaï P, Peyrusse O, Reverdin C, Soullié G, Tikhonchuk V, Villette B and Fourment C, Physical Review Letters. Vol. 98(9), pp. 095002.14  (2007). 
Abstract: Correct modeling of the electronenergy transport is essential for inertial confinement fusion target design. Various transport models have been proposed in order to extend the validity of a hydrodynamical description into weakly collisional regimes, taking into account the nonlocality of the electron transport combined with the effects of selfgenerated magnetic fields. We have carried out new experiments designed to be highly sensitive to the modeling of the heat flow on the Ligne d'Integration Laser facility, the prototype of the Laser Megajoule. We show that twodimensional hydrodynamic simulations correctly reproduce the experimental results only if they include both the nonlocal transport and magnetic fields. 
BibTeX:
@article{Schurtz2007, author = {Schurtz, G. and Gary, S. and Hulin, S. and ChenaisPopovics, C. and Gauthier, J.C. and Thais, F. and Breil, J. and Durut, J. and Feugeas, J.L. and Maire, P.H. and Nicolaï, P. and Peyrusse, O. and Reverdin, C. and Soullié, G. and Tikhonchuk, V. and Villette, B. and Fourment, C.}, title = {Revisiting nonlocal electronenergy transport in inertialfusion conditions}, journal = {Physical Review Letters}, year = {2007}, volume = {98}, number = {9}, pages = {095002.14}, url = {http://dx.doi.org/10.1103/PhysRevLett.98.095002}, doi = {10.1103/PhysRevLett.98.095002} } 
"Two CollisionalRadiative Codes based on the HULLAC suite: Detailed Levels (CRCHDL5) and Configuration Average (CRCHCA5)" Poirier M, In 5th NonLTE Code Comparison Workshop. EtatsUnis  (2007). [BibTeX] 
BibTeX:
@inproceedings{InproPoirier2007, author = {Poirier, M.}, title = {Two CollisionalRadiative Codes based on the HULLAC suite: Detailed Levels (CRCHDL5) and Configuration Average (CRCHCA5)}, booktitle = {5th NonLTE Code Comparison Workshop  2007}, year = {2007} } 
"Physique atomique des plasmas hors équilibre : codes détaillés et moyennes en configurations" Poirier M, de Gaufridy de Dortan F, Blenski T, Piron R and Thais F, In Forum ILP France  (2007). 
Abstract: Les plasmas créés en laboratoire, par exemple par interaction laser, ou ceux d'intérêt astrophysique sont souvent hors équilibre thermodynamique local. Les codes collisionnelsradiatifs (CR) permettent alors de caractériser ces plasmas et de décrire notamment leur distribution de charges, de populations, leur émissivité ou leur opacité. Après une brève revue des processus physiques mis en jeu et des modèles disponibles, deux codes CR fondés sur la suite HULLAC sont présentés, l'un détaillé et l'autre moyenné en configurations. Cette moyenne améliore considérablement la rapidité du calcul, cependant il est important de tester sa validité. Aussi un nouveau critère fondé sur le principe de microréversibilité estil proposé. Il est testé dans le cas d'un plasma de carbone et se révèle préférable au critère intuitif requérant que la moyenne de la dispersion en énergie des configurations soit plus petite que l'énergie thermique des électrons. Les améliorations possibles du modèle numérique et les applications nouvelles sont discutées. 
BibTeX:
@inproceedings{InproPoirier22007, author = {Poirier, M. and de Gaufridy de Dortan, F. and Blenski, T.J. and Piron, R. and Thais, F.}, title = {Physique atomique des plasmas hors équilibre : codes détaillés et moyennes en configurations}, booktitle = {Forum ILP  2007}, year = {2007} } 
2006 
"Interaction of intense VUV impulsions with luminescent solids." Belsky A, Carre B, N F, E F, Gaudin J, Guizard S, Geoffroy G, Grazia D, Kirm, Martin P, Merdji H, Nagirnyi, Petite G and Vasil'ev , Journal de Physique IV. Vol. 138, pp. 155161  (2006). 
Abstract: Nous présentons les résultats d'études de luminescence résolue en temps émise par des cristaux sous excitation par des photons VUV issus de la génération d'harmoniques d'ordre élevé. L'utilisation d'un laser TiSa PLFA à Saclay, qui délivre des impulsions d'une énergie de 13mJ et d'une durée de 35 fs à 1 KHz, pour la génération des harmoniques dans l'Argon et la microfocalisation du faisceau VUV nous ont permis de faire varier la densité du rayonnement sur la cible dans une large gamme. Nous avons étudié l'effet de la densité d'excitation VUV sur la luminescence intrinsèque de cristaux à large bande interdite (CdWO_{4} et BaF_{2}). En fonction de la densité d'excitation VUV nous avons observé les modifications des spectres d'émission et de la cinétique de la luminescence excitonique. Quand la densité d'excitation VUV croÃ®t, le rendement de la luminescence diminue et apparaissent dans la cinétique de luminescence descomposantes rapides. Le profil de la courbe de déclin devient alors complexe avec une forte déviation de la loi exponentielle dans sa partie initiale. 
BibTeX:
@article{Belsky2006, author = {Belsky, A. and Carre, B. and Fedorov N and Feldbach E and Gaudin, J. and Guizard, S. and Geoffroy, G. and De Grazia and Kirm and Martin, P. and Merdji, H. and Nagirnyi and Petite, G. and Vasil'ev}, title = {Interaction of intense VUV impulsions with luminescent solids.}, journal = {Journal de Physique IV}, year = {2006}, volume = {138}, pages = {155161}, url = {http://jp4.journaldephysique.org/articles/jp4/abs/2006/07/jp4138018/jp4138018.html}, doi = {10.1051/jp4:2006138018} } 
"On the linear dynamic response of average atom in plasma" Blenski T, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 99(13), pp. 84101  (2006). 
Abstract: The theory of linear response of an Average Atom (AA) in plasma is considered. It is assumed that the model of the AA is of the Density Functional Theory (DFT) type, i.e., can be characterized by an equilibrium electron density in terms of a complete set of bound and free oneelectron wave functions of a screened selfconsistentfield (SCF) potential. The starting point in the linear response theory is the cluster expansion of the energy extinction coefficient. This coefficient expresses the rate of extinction of the energy due to an external potential irradiating a plasma composed if ions and electrons. As shown in previous publications the first order term in the cluster expansion correctly gives the linear response of the AA. The first order formula for the extinction coefficient is directly related to the AA photoabsorption crosssection. The cluster expansion technique shows how the homogeneous plasma contribution shall be correctly subtracted from the response of the AA and its surrounding plasma. The linear response is considered in the dipole approximation and in the framework of the RPA approximation which can be viewed as a version of a timedependent DFT with local density approximation to the exchangecorrelation potential. In the paper we discuss a possible practical scheme for calculation of the dipole linear response and obtain some theoretical results that allow one to reduce the theoretical and numerical difficulties of the approach. We show formally how in the dipole approximation the homogeneous plasma contribution to the induced potential results in the appearance of the coldplasma dielectric function. We also derive a new sum rule which allows one to calculate the induced dipole using the localized density and potential gradients of the AA in equilibrium. We further propose a change of variables that allows us to eliminate the leading dipole divergence in the first order SchrÃ¶dinger equations. We next discuss some aspects of a simplified case in which the induced potential is neglected. Finally, we present and comment on the radial equations for the SCF frequencydependent induced density and potential. 
BibTeX:
@article{Blenski2006, author = {Blenski, T.}, title = {On the linear dynamic response of average atom in plasma}, journal = {Journal of Quantitative Spectroscopy and Radiative Transfer}, year = {2006}, volume = {99}, number = {13}, pages = {84101}, url = {http://dx.doi.org/10.1016/j.jqsrt.2005.05.007}, doi = {10.1016/j.jqsrt.2005.05.007} } 
"Use of luminescent materials for the metrology of intense UVX bundles of ultrashort impulsions." Fedorov, Nagirnyi, Vasil'ev, Belsky A, Carre B, Feldbach, Gaudin J, Geoffroy G, Guizard S, De Grazia M, Kirm M, Martin P, Merdji H and Petite G, Journal de Physique IV. Vol. 138, pp. 251257  (2006). 
Abstract: Récemment nous avons débuté des séries d'expériences sur l'interaction d'impulsions intenses VUV avec les solides luminescents. Le but principal en est l'étude des mécanismes d'interaction et de transfert d'énergie entre les excitations électroniques dans les solides à large bande interdite. L'application directe de ces études sera le développement de matériaux et de méthodes de métrologie pour les faisceauxUVX intenses. Nous présentons les résultats obtenus pour CdWO4 qui montrent que ce cristal pourra servir comme un scintillateur pour le rayonnement VUV intense. 
BibTeX:
@article{Fedorov2006, author = {Fedorov and Nagirnyi and Vasil'ev and Belsky, A. and Carre, B. and Feldbach and Gaudin, J. and Geoffroy, G. and Guizard, S. and De Grazia, M and Kirm, M.) and Martin, P. and Merdji, H. and Petite, G.}, title = {Use of luminescent materials for the metrology of intense UVX bundles of ultrashort impulsions.}, journal = {Journal de Physique IV}, year = {2006}, volume = {138}, pages = {251257}, url = {10.1051/jp4:2006138029} } 
"Astrophysical radiative shocks: From modeling to laboratory experiments" Gonzalez M, Stehlé C, Audit E, Busquet M, Rus B, Thais F, Acef O, Barroso P, BarShalom A, Bauduin D, Kozlova M, Lery T, Madouri A, Mocek T and Polan J, Laser and Particle Beams. Vol. 24, pp. 535540  (2006). 
Abstract: Radiative shock waves are observed around astronomical objects in a wide variety of environments, for example, they herald the birth of stars and sometimes their death. Such shocks can also be created in the laboratory, for example, by using energetic lasers. In the astronomical case, each observation is unique and almost fixed in time, while shocks produced in the laboratory and by numerical simulations can be reproduced, and investigated in greater detail. The combined study of experimental and computational results, as presented here, becomes a unique and powerful probe to understanding radiative shock physics. Here we show the first experiment on radiative shock performed at the PALS laser facility. The shock is driven by a piston made from plastic and gold in a cell filled with xenon at 0.2 bar. During the first 40 ns of the experiment, we have traced the radiative precursor velocity, that is showing a strong decrease at that stage. Threedimensional (3D) numerical simulations, including stateofart opacities, seem to indicate that the slowing down of the precursor is consistent with a radiative loss, induced by a transmission coefficient of about 60% at the walls of the cell. We infer that such 3D radiative effects are governed by the lateral extension of the shock wave, by the value of the opacity, and by the reflection on the walls. Further investigations will be required to quantify the relative importance of each component on the shock properties. 
BibTeX:
@article{Gonzalez2006, author = {Gonzalez, M. and Stehlé, C. and Audit, E. and Busquet, M. and Rus, B. and Thais, F. and Acef, O. and Barroso, P. and BarShalom, A. and Bauduin, D. and Kozlova, M. and Lery, T. and Madouri, A. and Mocek, T. and Polan, J.}, title = {Astrophysical radiative shocks: From modeling to laboratory experiments}, journal = {Laser and Particle Beams}, year = {2006}, volume = {24}, pages = {535540}, url = {http://dx.doi.org/10.1017/S026303460606071X}, doi = {10.1017/S026303460606071X} } 
"Quantum mechanical model for the study of pressure ionization in the superconfiguration approach" Pain J, Dejonghe G and Blenski T, Journal of Physics A. Mathematical and General Physics. Vol. 39, pp. 46594666  (2006). 
Abstract: The knowledge of plasma equation of state and photoabsorption requires suitable and realistic models for the description of ions. The number of relevant electronic configurations of ions in hot dense plasmas can be immense (increasing with atomic number Z). In such cases, calculations relying on the superconfiguration approximation appear to be among the best statistical approaches to photoabsorption in plasmas. The superconfiguration approximation enables one to perform rapid calculation of averages over all possible configurations representing excited states of bound electrons. We present a thermodynamically consistent model involving detailed screened ions (described by superconfigurations) in plasmas. The density effects are introduced via the ionsphere model. In the usual approaches, bound electrons are treated quantum mechanically while free electrons are described within the framework of semiclassical ThomasFermi theory. Such a hybrid treatment can lead to discontinuities in the thermodynamic quantities when pressure ionization occurs. We propose a model in which all electrons (bound and free) are treated quantum mechanically. Furthermore, resonances are carefully taken into account in the selfconsistent calculation of the electronic structure of each superconfiguration. The model provides the contribution of electrons to the main thermodynamic quantities, together with a treatment of pressure ionization, and gives a better insight into the electronic properties of hot dense plasmas. 
BibTeX:
@article{Pain2006, author = {Pain, J.C. and Dejonghe, G. and Blenski, T.J.}, title = {Quantum mechanical model for the study of pressure ionization in the superconfiguration approach}, journal = {Journal of Physics A. Mathematical and General Physics}, year = {2006}, volume = {39}, pages = {46594666}, url = {http://dx.doi.org/10.1088/03054470/39/17/S53}, doi = {10.1088/03054470/39/17/S53} } 
"A selfconsistent model for the study of electronic properties of hot dense plasmas in the superconfiguration approximation" Pain JC, Dejonghe G and Blenski T, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 99(13), pp. 451468  (2006). 
Abstract: We propose a thermodynamically consistent model involving detailed screened ion, described by superconfigurations, in plasmas. In the present work, the electrons, bound and free, are treated quantummechanically so that resonances are carefully taken into account in the selfconsistent calculation of the electronic structure of each superconfiguration. The procedure is in some sense similar to the one used in Inferno code develop by D. Liberman; however, here we perform this calculation in the ionsphere model for each superconfiguration. The superconfiguration approximation allows rapid calculation of necessary averages over all possible configurations representing excited states of bound electrons. The model enables a fully quantum mechanical selfconsistent calculation of the electronic structure of ions and provides the relevant thermodynamic quantities (e.g., internal energy, Helmholtz free energy and pressure), together with an improved treatment of pressure ionization. It should therefore give a better insight into the impact of plasma effects on photoabsorption spectra 
BibTeX:
@article{Pain2006a, author = {Pain, J.C. and Dejonghe, G. and Blenski, T.}, title = {A selfconsistent model for the study of electronic properties of hot dense plasmas in the superconfiguration approximation}, journal = {Journal of Quantitative Spectroscopy and Radiative Transfer}, year = {2006}, volume = {99}, number = {13}, pages = {451468}, url = {http://dx.doi.org/10.1016/j.jqsrt.2005.05.036}, doi = {10.1016/j.jqsrt.2005.05.036} } 
"Modeling of EUV emission from xenon and tin plasma sources for nanolithography" Poirier M, Blenski T, de Gaufridy de Dortan F and Gilleron F, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 99(13), pp. 482492  (2006). 
Abstract: Since the last decade a strong effort has been devoted to the development of efficient extreme UV sources designed for nanolithography, operating mainly in the 13.5 nm range. Possible devices involve laserproduced plasmas and dischargeproduced plasmas. This paper, devoted to the modeling of such emission, puts emphasis on the atomic physics effects and noticeably on configuration interaction. Mainly two types of theoretical approaches are presented, one involving the detailed computation with the parametric potential code HULLAC, the other based on the supraconfiguration code SCO. Computations of emission spectra in xenon and tin are presented. The possible influence of nonlocal thermodynamic equilibrium (LTE) effects is investigated using populations given by the simple collisionalradiative formulae from Colombant and Tonon. Convergence to LTE is analyzed in the tin case. 
BibTeX:
@article{Poirier2006, author = {Poirier, M. and Blenski, T. and de Gaufridy de Dortan, F. and Gilleron, F.}, title = {Modeling of EUV emission from xenon and tin plasma sources for nanolithography}, journal = {Journal of Quantitative Spectroscopy and Radiative Transfer}, year = {2006}, volume = {99}, number = {13}, pages = {482492}, url = {http://dx.doi.org/10.1016/j.jqsrt.2005.05.038}, doi = {10.1016/j.jqsrt.2005.05.038} } 
"Modeling laserproduced plasma sources" AlRabban M, Richardson M, Scott H, Gilleron F, Poirier M and Blenski T, In EUV Sources for Lithography. Vol. PM149, pp. 299337  (2006). 
BibTeX:
@incollection{InCollection2006, author = {AlRabban, M. and Richardson, M. and Scott, H. and Gilleron, F. and Poirier, M. and Blenski, T.J.}, editor = {V., Bakshi and Press, SPIE}, title = {Modeling laserproduced plasma sources}, booktitle = {EUV Sources for Lithography}, year = {2006}, volume = {PM149}, pages = {299337}, url = {http://bookstore.spie.org/index.cfm?fuseaction=DetailVolume&productid=613774} } 
"Interpretation of some X and XUV absorption experiments using the superconfiguration code SCO" Arnault P, Blenski T and Dejonghe G, In 12th International Workshop on Radiative Properties of Hot Dense Matter (RPHDM  2006). Portugal  (2006). [BibTeX] 
BibTeX:
@inproceedings{InproArnault2006, author = {Arnault, P. and Blenski, T.J. and Dejonghe, G.}, title = {Interpretation of some X and XUV absorption experiments using the superconfiguration code SCO}, booktitle = {12th International Workshop on Radiative Properties of Hot Dense Matter (RPHDM  2006)}, year = {2006} } 
"Measurement of XUV absorption spectra of ZnS radiatively heated foils" BastianiCeccotti S, Thais F, Kontogiannopoulos N, ChenaisPopovics C, Sauvan P, Schott R, Folsner W, Arnault P, Poirier M and Blenski T, In 12th International Workshop on Radiative Properties of Hot Dense Matter (RPHDM  2006). Portugal  (2006). [BibTeX] 
BibTeX:
@inproceedings{InproCeccotti2006, author = {BastianiCeccotti, S. and Thais, F. and Kontogiannopoulos, N. and ChenaisPopovics, C. and Sauvan, P. and Schott, R. and Folsner, W. and Arnault, P. and Poirier, M. and Blenski, T.J.}, title = {Measurement of XUV absorption spectra of ZnS radiatively heated foils}, booktitle = {12th International Workshop on Radiative Properties of Hot Dense Matter (RPHDM  2006)}, year = {2006} } 
"A variational approach to average atom and superconfigurations in plasmas" Blenski T and Cichocki B, In 12th International Workshop on Radiative Properties of Hot Dense Matter (RPHDM  2006). Portugal  (2006). [BibTeX] 
BibTeX:
@inproceedings{InproBlenski2006, author = {Blenski, T.J. and Cichocki, B.}, title = {A variational approach to average atom and superconfigurations in plasmas}, booktitle = {12th International Workshop on Radiative Properties of Hot Dense Matter (RPHDM  2006)}, year = {2006} } 
2005 
"Photoconductivité et photoémission de diamant(s) sous irradiation XUV femtoseconde" Gaudin J, Geoffroy G, Guizard S, Esnouf S, Olevano V, Petite G, Klimentov S, Pivovarov P, Garnov S, Carre B, Martin P and Belsky A, Journal de Physique IV. Vol. 127, pp. 131137  (2005). 
Abstract: Notamment à cause de ses applications à la détection rapide de particules, mais aussi parce qu'il représente un modèle de matériau covalent à grande bande interdite, se prêtant bien à la modélisation, l'étude du comportement des porteurs libres dans le diamant est un sujet particulièrement captivant. Nous avons abordé cette question sur le plan expérimental par une étude des propriétés de photoconductivité induite dans différents types de diamants (monocristaux de type IIa et couches CVD) par des impulsions femtosecondes allant du proche IR (800 nm) à l'XUV (jusqu'à l'harmonique 19 du laser titane/saphir). En complément de ces études, les spectres de photoémission de ces échantillons ont aussi été étudiés. La méthode utilisée pour la mesure de la photoconductivité est spécifique dans la mesure ou elle ne nécessite pas la réalisation de contacts ohmiques (mesure Â« capacitive Â» du courant de déplacement), et est donc d'une grande simplicité, et aussi d'une grande sensibilité (typiquement 1011 porteurs).Pour l'IR et les harmoniques basses du laser titane/saphir, on observe que la photoconductivité induite est essentiellement pilotée par les défauts du matériau : comportement linéaire en intensité dans la plupart des cas, forte sensibilité au chargement électronique des défauts dans le diamant CVD, au contraire de ce qui se passe dans un diamant pur. Des études en RPE menées sur les différents échantillons n'ont pas permis d'identifier clairement le défaut responsable, mais permettent par contre d'éliminer le centre P1. Une expérience est en cours pour étudier un matériau pur dans lequel des défauts lacunaires sont introduits par irradiation aux électrons de 2.5 MeV. On ne retrouve pas un telle sensibilité aux défauts quand on utilise les harmoniques élevées (7 et plus). Nous avons étudié le comportement du signal de photoconductivité en fonction de l'ordre de l'harmonique. Malgré des difficultés de calibration, on constate que ce signal augmente tout d'abord, avec l'ordre (harmoniques 9 à 13) puis diminue au delà. Si l'augmentation s'interprête aisément comme résultant de phénomènes de multiplication par collisions inélastiques, la diminution ultérieure n'a pas pour le moment d'explication. Les mesures de spectre et de rendement de photoémission permettent en effet d'exclure la compétition en photoconductivité et photoémission (l'excitation étant localisée dans ce cas près de la surface).Enfin, nous avons réalisé le premier calcul abinitio de la durée de vie des porteurs tenant compte des interactions électronélectron, à l'aide d'une approche de théorie quantique à plusieurs corps de type GW. Au voisinage du gap, on observe un comportement très proche de celui d'un liquide de Fermi (ce qui peut se comprendre ici aussi à l'aide d'arguments du type espace de phase accessible, mais qui néglige l'interaction électronphonon, importante dans cette gamme d'énergie). A plus haute énergie on observe des déviations à ce comportement, provenant d'effets de structure de bande d'une part, et d'excitations de plasmons d'autre part.Ce travail a été soutenu par le contrat INTAS 01458, ainsi que par le PAI FranceRussie nÂ° 04527 ZM. 
BibTeX:
@article{Gaudin2005a, author = {Gaudin, J. and Geoffroy, G. and Guizard, S. and Esnouf, S. and Olevano, V. and Petite, G. and Klimentov, S.M. and Pivovarov, P.A. and Garnov, S.V. and Carre, B. and Martin, P. and Belsky, A.}, title = {Photoconductivité et photoémission de diamant(s) sous irradiation XUV femtoseconde}, journal = {Journal de Physique IV}, year = {2005}, volume = {127}, pages = {131137}, url = {http://dx.doi.org/10.1051/jp4:2005127020} } 
"Plasmon channels in the electronic relaxation of diamond under highorder harmonics femtosecond irradiation." Gaudin J, Geoffroy G, Guizard S, Olevano V, Esnouf S, Klimentov S, Pivovarov P, Garnov S, Martin P, Belsky A and Petite G, Laser Physics Letters. Vol. 2(6), pp. 292296  (2005). 
Abstract: We used high order harmonics of a femtosecond titaniumdoped sapphire system (pulse duration 25 fs) to realise Ultraviolet Photoelectron Spectroscopy (UPS) measurements on diamond. The UPS spectra were measured for harmonics in the range 13 to 27. We also made ab initio calculations of the electronic lifetime of conduction electrons in the energy range produced in the UPS experiment. Such calculations show that the lifetime suddenly diminishes when the conduction electron energy reaches the plasmon energy, whereas the UPS spectra show evidence in this range of a strong relaxation mechanism with an increased production of low energy secondary electrons. We propose that in this case the electronic relaxation proceeds in two steps : excitation of a plasmon by the high energy electron, the latter decaying into individual electronhole pairs, as in the case of metals. This process is observed for the first time in an insulator and, on account of its high efficiency, should be introduced in the models of laser breakdown under high intensity. 
BibTeX:
@article{Gaudin2005, author = {Gaudin, J. and Geoffroy, G. and Guizard, S. and Olevano, V. and Esnouf, S. and Klimentov, S.M. and Pivovarov, P.A. and Garnov, S. and Martin, Pa. and Belsky, A. and Petite, G.}, title = {Plasmon channels in the electronic relaxation of diamond under highorder harmonics femtosecond irradiation.}, journal = {Laser Physics Letters}, year = {2005}, volume = {2}, number = {6}, pages = {292296}, url = {http://arxiv.org/abs/condmat/0501687}, doi = {10.1002/lapl.200510001} } 
"Timeresolved twocolour photoemission in wide band gap dielectrics" Guizard S, Belsky A, Gaudin J, Geoffroy G, Martin P, Petite G, Philippov A and Yatsenko B, Physica Status Solidi C  Current Topics in Solid State Physics. Vol. 2, pp. 223227  (2005). 
Abstract: We have measured the relaxation of photoexcited carriers in different wide band gap dielectrics by using time resolved twocolour photoemission. Electrons are excited by an ultrashort pulse of VUV photons directly in the conduction band. They are then are reexcited by an IR probe pulse. The evolution of the photoemission spectra as a function of the pumpprobe delay gives direct information on the relaxation of the population of excited electron. (Â© 2005 WILEYVCH Verlag GmbH & Co. KGaA, Weinheim) 
BibTeX:
@article{Guizard2005, author = {Guizard, S. and Belsky, A.N. and Gaudin, J. and Geoffroy, G. and Martin, Pa. and Petite, G. and Philippov, A. and Yatsenko, B.}, title = {Timeresolved twocolour photoemission in wide band gap dielectrics}, journal = {Physica Status Solidi C  Current Topics in Solid State Physics}, year = {2005}, volume = {2}, pages = {223227}, url = {http://www3.interscience.wiley.com/cgibin/abstract/109866909/ABSTRACT}, doi = {10.1002/pssc.200460151} } 
"Mesure de coefficients d'absorption de plasmas créés par laser nanoseconde" Thais F, ChenaisPopovics C, Eidmann K, Bastiani S, Blenski T and Gilleron F, Journal de Physique IV. Vol. 127, pp. 119124  (2005). 
Abstract: La mesure des coefficients d'absorption dans les plasmas chauds est particulièrement utile dans le domaine de la fusion par confinement inertiel ainsi que dans divers contextes en astrophysique. Le développement des calculs de physique atomique qui y sont associés repose sur des hypothèses qu'il est nécessaire de vérifier dans la plus large gamme possible de conditions physiques. Nous présentons ici la méthode de mesure et d'analyse employée en nous appuyant sur l'exemple des cibles multicouches nickel/aluminium. 
BibTeX:
@article{Thais2005, author = {Thais, F. and ChenaisPopovics, C. and Eidmann, K. and Bastiani, S. and Blenski, T. and Gilleron, F.}, title = {Mesure de coefficients d'absorption de plasmas créés par laser nanoseconde}, journal = {Journal de Physique IV}, year = {2005}, volume = {127}, pages = {119124}, url = {http://dx.doi.org/10.1051/jp4:2005127018}, doi = {10.1051/jp4:2005127018} } 
"Creation of high energy electronic excitations in inorganic insulators by intense femtosecond laser pulses" Yatsenko BN, Bachau H, Belsky AN, Gaudin J, Geoffroy G, Guizard S, Martin P, Petite G, Philippov A and Vassil'ev AN, Physica Status Solidi C  Current Topics in Solid State Physics. Vol. 2, pp. 240243  (2005). 
Abstract: We measured photoemission spectra for a number of insulators (CsI, Diamond, SiO_{2}, CeF_{3}) excited by femtosecond TiSapphire laser pulses at peak intensities, from 0.5 to 6 TW/cm^{2}, which are at least one order of magnitude below the optical breakdown threshold. An intense and pronounced plateau of high energy electrons appears in the photoelectron spectra in this intensity range, which extends up to 3040 eV at the highest intensities, which we used. The excitation of electrons at high energies is treated in terms of direct interbranch transitions in the conduction band of insulator. These processes are described using calculations based on numerical solution of time dependant SchrÃ¶dinger equation (TDSE) for Bloch electrons in electric fields. (Â© 2005 WILEYVCH Verlag GmbH & Co. KGaA, Weinheim) 
BibTeX:
@article{Yatsenko2005, author = {Yatsenko, B. N. and Bachau, H. and Belsky, A. N. and Gaudin, J. and Geoffroy, G. and Guizard, S. and Martin, P. and Petite, G. and Philippov, A. and Vassil'ev, A. N.}, title = {Creation of high energy electronic excitations in inorganic insulators by intense femtosecond laser pulses}, journal = {Physica Status Solidi C  Current Topics in Solid State Physics}, year = {2005}, volume = {2}, pages = {240243}, url = {http://www3.interscience.wiley.com/cgibin/abstract/109866894/ABSTRACT}, doi = {10.1002/pssc.200460155} } 
"Température radiative de cavités chauffées avec le laser NANO 2000" ChenaisPopovics C, Tzortzakis S, Bastiani S, Radier C, Chiaramonti B, Thais F, Eidmann K and Foelsner W, pp.3 pages  (2005). 
Abstract: Absorption coefficients of hot dense matter in local thermodynamic equilibrium can be measured in a foil radiatively heated by the Xray emission of a laser heated cavity. The present measurements provide the radiative temperature of a 1.2 mm diameter gold cavity. The laser beam isdirectly focused inside the cavity or heats a thin gold foil set on the cavity entrance hole. The radiative temperature is in the range of 90100 eV for both types of cavities. 
BibTeX:
@techreport{Techreport2005, author = {ChenaisPopovics, C. and Tzortzakis, S. and Bastiani, S. and Radier, C. and Chiaramonti, B. and Thais, F. and Eidmann, K. and Foelsner, W.}, title = {Température radiative de cavités chauffées avec le laser NANO 2000}, year = {2005}, pages = {3 pages} } 
"Selfconsistent statistical approach to electronic properties of hot dense plasmas" Pain JC, Dejonghe G and Blenski T, In Conference on "Strongly Coupled Coulomb Systems". Moscou  (2005). [BibTeX] 
BibTeX:
@inproceedings{InproPain2005, author = {Pain, J.C. and Dejonghe, G. and Blenski, T.}, title = {Selfconsistent statistical approach to electronic properties of hot dense plasmas}, booktitle = {Conference on "Strongly Coupled Coulomb Systems"}, year = {2005} } 
2004 
"Heating of Conduction Band Electrons by Intense Femtosecond Laser Pulses" Belsky A, Martin P, Bachau H, Vasil'ev A, Yatsenko B, Guizard S, Geoffroy G and Petite G, Europhysics Letters. Vol. 67, pp. 301306  (2004). 
Abstract: We present photoelectron spectra for CsI excited by intense femtosecond TiSapphire laser pulses. A high energy plateau is detected in the spectra, at excitation intensities above 0.5 TW/cmË›. This plateau extends up to 24 eV at 3 TW/cmË› and 90% of the emitted electrons have energy higher than twice the laser photon energy. Such intensive electron heating in solids can not be explained in terms of phonon assisted transitions. A model of conduction band electrons heating, which accounts for direct interbranch transitions in strong laser field, is used for simulation of photoelectron spectra 
BibTeX:
@article{Belsky2004b, author = {Belsky, A. and Martin, P. and Bachau, H. and Vasil'ev, A.N. and Yatsenko, B. and Guizard, S. and Geoffroy, G. and Petite, G.}, title = {Heating of Conduction Band Electrons by Intense Femtosecond Laser Pulses}, journal = {Europhysics Letters}, year = {2004}, volume = {67}, pages = {301306}, url = {http://iopscience.iop.org/02955075/67/2/301}, doi = {10.1209/epl/i2004100580} } 
"Observation of high energy photoelectrons from solids at moderate laser intensity" Belsky AN, Bachau H, Gaudin J, Geoffroy G, Guizard S, Martin P, Petite G, Philippov A, Vasil'ev AN and Yatsenko BN, Applied Physics B : Lasers and Optics. Vol. 78(78), pp. 989  (2004). 
Abstract: We investigate the photoemission for a set of wide bandgap crystals irradiated by femtosecond TiSapphire laser pulses at intensities varying from 0.5 to 6 TW/cm^{2} (below the optical breakdown threshold). The measured total electron yield increases linearly with the laser intensity in this intensity range. An intense and wide plateau of high energy electrons appears in the photoelectron spectra at excitation intensities larger than 1 TW/cm2. The exponential cutoff of this plateau reaches 40 eV at maximal applied intensities. In order to explain such a behavior, we propose a mechanism where the heating is due to a sequence of direct interbranch one and multiphoton transitions in the conduction band. 
BibTeX:
@article{Belsky2004, author = {Belsky, A.N. and Bachau, H. and Gaudin, J. and Geoffroy, G. and Guizard, S. and Martin, Ph. and Petite, G. and Philippov, A. and Vasil'ev, A.N. and Yatsenko, B.N.}, title = {Observation of high energy photoelectrons from solids at moderate laser intensity}, journal = {Applied Physics B : Lasers and Optics}, year = {2004}, volume = {78}, number = {78}, pages = {989}, url = {http://link.springer.com/article/10.1007%2Fs0034000414381#} } 
"Observation of laser driven supercritical radiative shock precursors" Bouquet S, Stehle C, Koenig M, Chieze J, BenuzziMounaix A, Batani D, Leygnac S, Fleury X, Merdji H, Michaut C, Thais F, Grandjouan N, Hall T, Henry E, Malka V and Lafon JP, Physical Review Letters. Vol. 92, pp. 225001  (2004). 
Abstract: We present a supercritical radiative shock experiment performed with the LULI nanosecond laser facility. Using targets filled with xenon gas at low pressure, the propagation of a strong shock with a radiative precursor is evidenced. The main measured shock quantities (electronic density and propagation velocity) are shown to be in good agreement with theory and numerical simulations. PACS numbers. 95.30.Jx, 52.72.+v 
BibTeX:
@article{Bouquet2004, author = {Bouquet, S. and Stehle, C. and Koenig, M. and Chieze, J.P. and BenuzziMounaix, A. and Batani, D. and Leygnac, S. and Fleury, X. and Merdji, H. and Michaut, C. and Thais, F. and Grandjouan, N. and Hall, T. and Henry, E. and Malka, V. and Lafon, JP.}, title = {Observation of laser driven supercritical radiative shock precursors}, journal = {Physical Review Letters}, year = {2004}, volume = {92}, pages = {225001}, url = {http://dx.doi.org/10.1103/PhysRevLett.92.225001}, doi = {10.1103/PhysRevLett.92.225001} } 
"Photoconductivity and photoemission studies of diamond irradiated by ultrashort VUV pulses" Gaudin J, Geoffroy G, Guizard S, Petite G, Klimentov S, Garnov S, Pivovarov P, Carré B, Belsky A and Martin P, Applied Physics B : Lasers and Optics. Vol. 78(78), pp. 10011004  (2004). 
Abstract: We investigated relaxation of free charge carriers in pure crystalline diamond exposed to VUV irradiation of high order harmonics of femtosecond Ti:Sa laser in the spectral range 1732 eV.Electronhole pairs, possessing a significant kinetic energy, are generated in the material via direct interband transitions possessing significant kinetic energy, relaxation of which is monitored by means of induced conductivity in the bulk and photoemission from the surface of the material.The experimental data provided by these complementary techniques are compared and discussed in terms of competition between ionization and conductivity looking for evidences of multiplication of free charge carriers due to impact ionization. 
BibTeX:
@article{Gaudin2004a, author = {Gaudin, J. and Geoffroy, G. and Guizard, S. and Petite, G. and Klimentov, S.M. and Garnov, S.V. and Pivovarov, P.A. and Carré, B. and Belsky, A. and Martin, P.}, title = {Photoconductivity and photoemission studies of diamond irradiated by ultrashort VUV pulses}, journal = {Applied Physics B : Lasers and Optics}, year = {2004}, volume = {78}, number = {78}, pages = {10011004}, url = {http://springerlink.metapress.com/app/home/contribution.asp?wasp=n49byglgxmcvydm38dwg&referrer=parent&backto=searcharticlesresults,1,2;journal,1,1;linkingpublicationresults,1:100502,1}, doi = {10.1007/s0034000414541} } 
"Absorption of LTE aluminum and nickel at different densities" BastianiCeccotti S, ChenaisPopovics C, Pisani F, Thais F, Gauthier JC, Gilleron F, Blenski T, Poirier M, Folsner W and Eidmann K, In Inertial Fusion Sciences and Applications 2003 (IFSA 2003). , pp. 987  (2004). [BibTeX] 
BibTeX:
@incollection{Incollection2004, author = {BastianiCeccotti, S. and ChenaisPopovics, C. and Pisani, F. and Thais, F. and Gauthier, J.C. and Gilleron, F. and Blenski, T. and Poirier, M. and Folsner, W. and Eidmann, K.}, editor = {Society, American Nuclear and Hammel, B.A. and Meyerhofen, D.D. and MeyerterVehn, Y. and Azechi, H.}, title = {Absorption of LTE aluminum and nickel at different densities}, booktitle = {Inertial Fusion Sciences and Applications 2003 (IFSA 2003)}, year = {2004}, pages = {987} } 
"Experimental characterization of electron densities and temperatures in radiative shocks" Leygnac S, Michaut C, Sthelé C, Vinci T, Koenig M, BenuzziMounaix A, Bouquet S, Thais F and Merdji H, In Third International Conference on Inertial Fusion Sciences and Applications (IFSA2003). EtatsUnis Vol. (7003), pp. 958  (2004). [BibTeX] 
BibTeX:
@inproceedings{InproLeygnac2004, author = {Leygnac, S. and Michaut, C. and Sthelé, C. and Vinci, T. and Koenig, M. and BenuzziMounaix, A. and Bouquet, S. and Thais, F. and Merdji, H.}, title = {Experimental characterization of electron densities and temperatures in radiative shocks}, booktitle = {Third International Conference on Inertial Fusion Sciences and Applications (IFSA2003)}, year = {2004}, volume = {(7003)}, pages = {958} } 
2003 
"Opacity measurements of tamped NaBr samples heated by zpinch Xrays" Bailey JE, Arnault P, Dejonghe G, Peyrusse O, MacFarlane JJ, Mancini RC, Cuneo ME, Nielsen DS, Rochau GA and Blenski T, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 81(14), pp. 3145  (2003). 
Abstract: Laboratory measurements provide benchmark data for wavelengthdependent plasma opacities to assist inertial confinement fusion, astrophysics, and atomic physics research. There are several potential benefits to using zpinch radiation for opacity measurements, including relatively large cmscale lateral sample sizes and relativelylong 3â€“ experiment durations. These features enhance sample uniformity. The spectrally resolved transmission through a CHtamped NaBr foil was measured. The zpinch produced the Xrays for both the heating source and backlight source. The (50Â±4) eV foil electron temperature and foil electron density were determined by analysis of the Na absorption features. LTE and NLTE opacity model calculations of the n=2 to 3, 4 transitions in bromine ionized into the Mshell are in reasonably good agreement with the data. 
BibTeX:
@article{Bailey2003, author = "J.E. Bailey and P. Arnault and T. Blenski and G. Dejonghe and O. Peyrusse and J.J. MacFarlane and R.C. Mancini and M.E. Cuneo and D.S. Nielsen and G.A. Rochau", title = "Opacity measurements of tamped NaBr samples heated by zpinch Xrays", journal = "Journal of Quantitative Spectroscopy and Radiative Transfer", volume = "81", number = "1", pages = "31  45", year = "2003", note = "Radiative Properties of Hot Dense Matter", issn = "00224073", doi = "10.1016/S00224073(03)000505", url = "http://www.sciencedirect.com/science/article/pii/S0022407303000505", } 
"Photoémission de CsI induite par une impulsion laser intense femtoseconde" Belsky A, Vasil'ev A, Yatsenko B, Bachau H, Martin P, Geoffroy G and Guizard S, Journal de Physique IV. Vol. 108, pp. 113117  (2003). 
Abstract: Nous avons mesuré pour la première fois les spectres de photoélectrons émis par un cristal isolant à large bande interdite, CsI, avec une dynamique de 106 coups/s, excité par la source laser haute cadence du C.E.L.I.A ( 800 nm, 40 fs, I kHz, 1 TW). L'émission d'électrons jusqu'à des énergies de quelques dizaines d'électronsvolts a été observée pour des impulsions d'éclairement compris entre 0.5 et 3 TW/cm2, relativement faible donc par comparaison aux éclairements utilisés pour accélérer les électrons d'un atome aux mêmes énergies. Ces spectres contiennent tous, en particulier, deux bandes dans le domaine des basses énergies d'électrons (<5 eV), également observées lors d'études précédentes. Les électrons les plus énergétiques forment un plateau intense légèrement structuré et limité par une coupure exponentielle. Pour des impulsions de 3 TW/cm2 cette coupure est située à 27 eV. L'insuffisance du mécanisme électronphotonphonon, considéré jusqu'à présent comme le principal processus d'échauffement des électrons dans les solides en interaction non destructrice avec un champ laser, nous a poussé à proposer un mécanisme alternatif. Ce modèle met en évidence les transitions directes multiphotoniques dans la bande de conduction du solide qui sont incontournables du fait de sa structure électronique multibranches. 
BibTeX:
@article{Belsky2003, author = {Belsky, A. and Vasil'ev, A.N. and Yatsenko, B. and Bachau, H. and Martin, P. and Geoffroy, G. and Guizard, S.}, title = {Photoémission de CsI induite par une impulsion laser intense femtoseconde}, journal = {Journal de Physique IV}, year = {2003}, volume = {108}, pages = {113117}, url = {http://cat.inist.fr/?aModele=afficheN&cpsidt=14859859} } 
"La photoémission VUV résolue en temps sur des solides isolants" Geoffroy G, Guizard S, Constant E, Mevel E, Belsky A and Martin P, Journal de Physique IV. Vol. 108, pp. 119122  (2003)  (2003). 
Abstract: L'objectif de ce travail expérimental est l'étude de la dynamique des processus de relaxations électroniques dans les solides, et en particulier dans les diélectriques. La technique la plus couramment employée pour étudier ces phénomènes est la photoémission résolue en temps, à l'aide d'impulsions laser ultrabrèves. Une première impulsion excite les électrons du solide, et une seconde impulsion provoque l'ionisation d'une partie de ces électrons. La mesure de l'énergie cinétique de ces photoélectrons en fonction du retard entre les impulsions pompe et sonde donne une image directe de l'évolution de leur distribution énergétique. Cette technique très puissance a déjà été utilisée pour étudier les cinétiques de relaxation dans les semiconducteurs et les métaux. En effet, les énergies de photons nécessaires aux excitations électroniques correspondent aux longueurs d'onde d'émission des lasers femtosecondes les plus courants. Les harmoniques d'ordres élevés obtenues à partir de laser femtosecondes intenses permettent d'étendre ces études à des matériaux isolants à grande bande interdite. Les résultats d'une étude systématique de la relaxation d'électrons de grande énergie (~30 eV) dans différents diélectriques (Si02, CeF3), réalisées avec la source d'harmoniques du laboratoire CELIA sont comparés et discutés. 
BibTeX:
@article{Geoffroy2003, author = {Geoffroy, G. and Guizard, S. and Constant, E. and Mevel, E. and Belsky, A. and Martin, P.}, title = {La photoémission VUV résolue en temps sur des solides isolants}, journal = {Journal de Physique IV}, year = {2003}, volume = {108}, pages = {119122}, url = {http://jp4.journaldephysique.org/articles/jp4/abs/2003/07/jp4pr6p119/jp4pr6p119.html}, doi = {10.1051/jp4:20030610} } 
"Emissive Properties of Xenon Ions from a LaserProduced Plasma in the 100140 Angström Spectral Range: AtomicPhysics Analysis of the Experimental Data" Gilleron F, Poirier M, Blenski T, Schmidt M and Ceccotti T, Journal of Applied Physics. Vol. 94(3), pp. 20862096  (2003). 
Abstract: In order to design extreme ultraviolet sources for nanolithography, xenon EUV emission has been experimentally studied in a plasma generated by the interaction of a highpower laser with a droplet jet. A theoretical model assuming that the resulting plasma is optically thick allows to find the distribution of the relevant ions and transitions involved in the emission process. Atomic physics computations are performed using the HULLAC code to give a detailed account of the transitions involved. The importance of 4p4d, 4d4f and 4d5p transitions is stressed, as well as the need for configurationinteraction treatment of the Delta n=0 transitions. Comparisons of a modeled LTE spectrum with experiment provides qualitative agreement and permits an estimate of the plasma temperature, density, and dimensions. 
BibTeX:
@article{Gilleron2003, author = {Gilleron, F. and Poirier, M. and Blenski, T. and Schmidt, M. and Ceccotti, T.}, title = {Emissive Properties of Xenon Ions from a LaserProduced Plasma in the 100140 Angström Spectral Range: AtomicPhysics Analysis of the Experimental Data}, journal = {Journal of Applied Physics}, year = {2003}, volume = {94}, number = {3}, pages = {20862096}, url = {http://dx.doi.org/10.1063/1.1587264}, doi = {http://jap.aip.org/resource/1/japiau/v94/i3/p2086_s1} } 
"A SANS investigation of the irradiationenhanced aâ€“a' phases separation in 7â€“12 Cr martensitic steels" Mathon M, de Carlan Y, Geoffroy G, Averty X, Alamo A and de Novion C, Journal of Nuclear Materials. Vol. 312, pp. 236248 (2003). 
Abstract: Five reduced activation (RA) and four conventional martensitic steels, with chromium contents ranging from 7 to 12 wt%, were investigated by small angle neutron scattering (SANS) under magnetic field after neutron irradiation (0.7â€“2.9 dpa between 250 and 400 Â°C). It was shown that when the Cr content of the b.c.c. ferritic matrix is larger than a critical threshold value ( ~ 7.2 at.% at 325 Â°C), the ferrite separates under neutron irradiation into two isomorphous phases, Ferich (a) and Crrich (a'). The kinetics of phase separation are much faster than under thermal aging. The quantity of precipitated a' phase increases with the Cr content, the irradiation dose, and as the irradiation temperature is reduced. The influence of Ta and W added to the RA steels seems negligible. Coldwork pretreatment increases slightly the coarsening of irradiationinduced precipitates in the 9Crâ€“1Mo (EM10) steel. In the case of the low Cr content F82H steel irradiated 2.9 dpa at 325 Â°C, where a' phase does not form, a small irradiationinduced SANS intensity is detected, which is probably due to point defect clusters. The a' precipitates contribute significantly to the irradiationinduced hardening of 9â€“12 wt% Cr content steels. 
BibTeX:
@article{Mathon2003, author = {Mathon, M.H. and de Carlan, Y. and Geoffroy, G. and Averty, X. and Alamo, A. and de Novion, C.H.}, title = {A SANS investigation of the irradiationenhanced aâ€“a' phases separation in 7â€“12 Cr martensitic steels}, journal = {Journal of Nuclear Materials}, year = {2003}, volume = {312}, pages = {236248}, url = {http://www.researchgate.net/publication/229391670_A_SANS_investigation_of_the_irradiationenhanced__phases_separation_in_712_Cr_martensitic_steels}, doi = {10.1016/S00223115(02)016306} } 
"Selfconsistent approach for the thermodynamics of ions in dense plasmas in the superconfiguration approximation" Pain JC and Blenski T, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 81(14), pp. 355369  (2003). 
Abstract: We propose a new thermodynamic approach to ions in dense plasmas taking into account the screening by free electrons. The ions in fundamental and excited states are represented by a group of superconfigurations. Each superconfiguration containing an integer number of bound electrons is totally screened by free electrons in a WignerSeitz (WS) sphere. The minimisation of the plasma free energy with respect to the WS radii of the ions, under the condition that the specific mass of the plasma is preserved, leads to the equality of the electronic pressure for all ions. This pressure, as well as the WS radii and the distribution of ionic probabilities, are calculated by iteration. In this way, our approach not only gives the charge neutrality of the plasma, but also assures that the plasma environment is the same for each ion. In principle, the proposed approach allows one to apply the superconfiguration method to calculate radiative properties of plasmas for higher densities than those encountered in transmission experiments. Numerical examples for nickel, aluminium and samarium plasmas will be given. Comparisons with results from the previous statistical approach using the same WS radius for each ion charge state will also be discussed. 
BibTeX:
@article{Pain2003, author = {Pain, J.Ch. and Blenski, T.}, title = {Selfconsistent approach for the thermodynamics of ions in dense plasmas in the superconfiguration approximation}, journal = {Journal of Quantitative Spectroscopy and Radiative Transfer}, year = {2003}, volume = {81}, number = {14}, pages = {355369}, url = {http://dx.doi.org/doi:10.1016/S00224073(03)000876}, doi = {10.1016/S00224073(03)000876} } 
"Absorption of local thermodynamic equilibrium aluminum at different densities" Thais F, Bastiani S, Blenski T, ChenaisPopovics C, Eidmann K, Folsner W, Gauthier JC, Gilleron F and Poirier M, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 81(14), pp. 473485  (2003). 
Abstract: Increasing the range of plasma parameters accessible for laboratory absorption coefficients measurements is of interest for astrophysical applications. Aluminum is of special interest as its 1s2p inner shell absorption transitions permit one to precisely determine the ionization balance that is strongly dependent on the electron temperature. A method to increase the density of the probed sample was tested on aluminum confined by carbon tampers of different thickness (8 to 70 Âµg/cm2). This created a density increase in the aluminum of a factor of ~10. Measurements showed that the aluminum ionization decreases substantially with increasing carbon thickness. Radiative hydrodynamic simulations showed that density and temperature gradients could not be neglected and had to be taken into account in calculating the absorption structures with the atomic physics code HULLAC. Very good agreement between theory and experiment was obtained by coupling HULLAC with hydrodynamic simulations. 
BibTeX:
@article{Thais2003, author = {Thais, F. and Bastiani, S. and Blenski, T. and ChenaisPopovics, C. and Eidmann, K. and Folsner, W. and Gauthier, J.C. and Gilleron, F. and Poirier, M.}, title = {Absorption of local thermodynamic equilibrium aluminum at different densities}, journal = {Journal of Quantitative Spectroscopy and Radiative Transfer}, year = {2003}, volume = {81}, number = {14}, pages = {473485}, url = {http://dx.doi.org/doi:10.1016/S00224073(03)000979}, doi = {10.1016/S00224073(03)000979} } 
"XUV emission from a xenon plasma: atomic physics models" Poirier M, Gilleron F, Blenski T, Schmidt M and Ceccotti T, In EUV Source Modeling Workshop. Anvers (Belgique)  (2003). 
Abstract: In this talk, various theoretical approaches are proposed in order to analyze the extremeUV emission from laserproduced xenon plasmas. In a first step, the superconfiguration code allows one to define the relevant ionic stages and the monoelectronic transitions involved. Then, an analysis using the relativistic parametric potential code HULLAC emphasizes the importance of configuration interaction (CI): while CI weakly affects the 4d5p lines in the 130140 Ä¹ region, it strongly shrinks the 4p4d and 4d4f lines which for the relevant ionic stages coalesce in the 100110 Ä¹ band. This analysis confirms the main importance of Xe 10+ ions in the 130140 Ä¹ range, but Xe 4+ appears as a new candidate for nanolithography since it exhibits an isolated line close to the 135 Ä¹ wavelength. Since various part of the experimental spectrum are most efficiently reproduced at various temperatures, the possibility of nonLTE effects is mentioned. The influence of doublyexcited states is stressed as well. Possible improvements of the theoretical description are finally reviewed. 
BibTeX:
@inproceedings{InproPoirier2003, author = {Poirier, M. and Gilleron, F. and Blenski, T. and Schmidt, M. and Ceccotti, T.}, title = {XUV emission from a xenon plasma: atomic physics models}, booktitle = {EUV Source Modeling Workshop}, year = {2003} } 
2002 
"Sur la physique atomique des ions dans les plasmas en présence de l'écrantage" Pain J  (2002). 
Abstract: Résumé : L'objectif de ce travail de thèse est d'améliorer la caractérisation des différentes espèces ioniques présentes dans les plasmas. La modélisation de la thermodynamique de ces plasmas est importante, notamment pour décrire leur capacité à absorber le rayonnement électromagnétique. L'écrantage des ions par les électrons libres joue un rôle capital dans cette thermodynamique. Le nombre de configurations électroniques du plasma est considérable, ce qui rend leur traitement détaillé prohibitif. Une approche récente fondée sur l'approximation des ''supraconfigurations'' permet de regrouper les configurations électroniques des ions en quelques centaines ou milliers de supraconfigurations pertinentes. Chaque supraconfiguration est caractérisée par un potentiel ainsi qu'une base d'états quantiques à un électron qui sont calculés de manière autocohérente. Ce travail de thèse constitue une amélioration de la méthode des supraconfigurations, prenant en compte l'écrantage des ions par les électrons délocalisés et assurant simultanément que chaque espèce ionique a le même environnement plasma. Ainsi, l'approche proposée assure non seulement la neutralité électrique du plasma, mais aussi, en faisant varier les volumes des sphères ioniques, l'égalité de la pression électronique du plasma autour de chaque ion. Cette égalité est obtenue par un calcul itératif fondé sur la méthode de Newton multidimensionnelle. Ce calcul est complexe mais la méthode converge et permet, dans le cas de plasmas de fortes densités (de l'ordre de la densité du solide), de mieux tenir compte de phénomènes d'ionisation par pression. L'impact de cette nouvelle approche thermodynamique sur le calcul de spectres de photoabsorption a été étudié. Des comparaisons avec des spectres expérimentaux obtenus au laboratoire LULI ont été effectuées. Une nouvelle règle de somme concernant la densité dipolaire induite a été obtenue dans le cadre d'une étude de la réponse linéaire prenant en compte l'écrantage dynamique dans les plasmas. This work is an improvement of the characterisation of ionic species in plasmas. It is important to model the thermodynamics of these plasmas, especially in order to describe their ability to absorb radiations. The screening of ions by free electrons plays a crucial role in these thermodynamics. The number of electronic configurations in the plasma is huge, which makes their individual treatment prohibitive. A recently developed approach based on the " superconfiguration " approximation enables to group electronic configurations into several hundreds or thousands of relevant superconfigurations. Each superconfiguration is characterised by a potential and a oneelectronquantumstate basis calculated in a selfconsistent way. The present work consists in a improvement of the superconfiguration method, in which the screening of ions by free electrons is taken into account and each ionic specie has the same plasma environment. Therefore, the proposed approach not only assures that the plasma is electrically neutral, by also gives, varying the volume of each ion sphere, the equality of the electronic pressure around each ion. This equality is obtained by a multidimensional Newton method. The latter calculation is complex but the method is definitely convergent and allows, in case of highdensity plasmas (about density of solids) to take pressure ionisation phenomena into account. The influence of the new thermodynamics on photoabsorption spectra has been studied. Comparisons with experimental spectra obtained in LULI laboratory have been investigated. In the framework of dynamic linear response theory, a new sum rule for the induced dipolar density has been developed. 
BibTeX:
@mastersthesis{pain2002, author = {Pain, J.}, title = {Sur la physique atomique des ions dans les plasmas en présence de l'écrantage} } 
"Lband xray absorption of radiatively heated nickel" ChenaisPopovics C, Fajardo M, Gilleron F, Teubner U, Gauthier JC, BaucheArnoult C, Bachelier A, Bauche J, Blenski T, Thais F, Perrot F, Benuzzi A, TurckChieze S, Chieze JP, Dorchies F, Andiel U, Foelsner W and Eidmann K, Physical Review E  Statistical, Nonlinear, and Soft Matter Physics. Vol. 65(1), pp. 016413/19  (2002). 
Abstract: Absorption of LM and LN transitions of nickel has been measured using point projection spectroscopy. The xray radiation from laserirradiated gold cavities was used to heat volumetrically nickel foils "tamped with carbon" up to 20 eV. Experimental spectra have been analyzed with calculations based on the spinorbit split arrays statistical approach and performed for each ionic species Ni 5+ to Ni 11+ . Using a leastsquares fit, this method provides an ion distribution broader than at local thermodynamic equilibrium, which is explained by spatial and temporal temperature gradients. A major improvement in the simulation of the absolute value of transmission is obtained with a resolved transition array statistical calculation that reproduces the experimental spectrum with the nominal areal mass density by taking into account the saturation of narrow lines. 
BibTeX:
@article{ChenaisPopovics2002, author = {ChenaisPopovics, C. and Fajardo, M. and Gilleron, F. and Teubner, U. and Gauthier, J.C. and BaucheArnoult, C. and Bachelier, A. and Bauche, J. and Blenski, T. and Thais, F. and Perrot, F. and Benuzzi, A. and TurckChieze, S. and Chieze, J.P. and Dorchies, F. and Andiel, U. and Foelsner, W. and Eidmann, K.}, title = {Lband xray absorption of radiatively heated nickel}, journal = {Physical Review E  Statistical, Nonlinear, and Soft Matter Physics}, year = {2002}, volume = {65}, number = {1}, pages = {016413/19}, url = {http://link.aps.org/abstract/PRE/v65/e016413}, doi = {10.1103/PhysRevE.65.016413} } 
"A laser experiment for studying radiative shocks in astrophysics" Fleury X, Bouquet S, Stehlé C, Koenig M, Batani D, BenuzziMounaix A, Chièze JP, Grandjouan N, Grenier J, Hall T, Henry E, Lafon JP, Leygnac S, Malka V, Marchet B, Merdji H, Michaut C and Thais F, Laser and Particle Beams. Vol. 20(2), pp. 263  (2002); 
Abstract: In this article, we present a laboratory astrophysics experiment on radiative shocks and its interpretation using simple modelization. The experiment is performed with a 100J laser (pulse duration of about 0.5 ns) which irradiates a 1mm 3 xenon gasfilled cell. Descriptions of both the experiment and the associated diagnostics are given. The apparition of a radiation precursor in the unshocked material is evidenced from interferometry diagrams. A model including selfsimilar solutions and numerical ones is derived and fairly good agreements are obtained between the theoretical and the experimental results. 
BibTeX:
@article{Fleury2002, author = {Fleury, X. and Bouquet, S. and Stehlé, C. and Koenig, M. and Batani, D. and BenuzziMounaix, A. and Chièze, J.P. and Grandjouan, N. and Grenier, J. and Hall, T. and Henry, E. and Lafon, J.P. and Leygnac, S. and Malka, V. and Marchet, B. and Merdji, H. and Michaut, C. and Thais, F.}, title = {A laser experiment for studying radiative shocks in astrophysics}, journal = {Laser and Particle Beams}, year = {2002}, volume = {20}, number = {2}, pages = {263}, url = {http://journals.cambridge.org/bin/bladerunner?REQUNIQ=1065531404&REQSESS=16896055&117000REQEVENT=&REQINT1=130342&REQAUTH=0}, doi = {10.1017/S0263034602202165} } 
"Des étoiles en laboratoire" Merdji H and Thais F, Phases Magazine, La lettre du DRECAM et du SPhT. Vol. 119, pp. 1  (2002). [BibTeX] 
BibTeX:
@article{Merdji2002, author = {Merdji, H. and Thais, F.}, title = {Des étoiles en laboratoire}, journal = {Phases Magazine, La lettre du DRECAM et du SPhT}, year = {2002}, volume = {119}, pages = {1} } 
"New approach to dense plasma thermodynamics in the superconfiguration approximation" Pain JC and Blenski T, Laser and Particle Beams. Vol. 20(2), pp. 211216  (2002). 
Abstract: We propose a new approach to the calculation of ion populations in the LTE dense plasmas in the superconfiguration approximation. The screening of plasma ions is obtained using the same freeelectron chemical potential for each ion charge. This chemical potential is determined by iteration keeping the total density constant and varying the volume of each ion. In such a way our approach not only gives the charge neutrality of the plasma, but also assures that the freeelectron density is equal in the vicinity of each ion. The resulting ion charge distribution is different with respect to the one obtained without imposing the constraint of equal chemical potential. For instance, the effective charge is a little bit higher, which can change the shape of the absorption spectra, especially at higher densities. Examples of absorption spectra of mediumZ plasmas in a temperature and density range close to the present opacity measurements are shown. 
BibTeX:
@article{Pain2002, author = {Pain, J.Ch. and Blenski, T.}, title = {New approach to dense plasma thermodynamics in the superconfiguration approximation}, journal = {Laser and Particle Beams}, year = {2002}, volume = {20}, number = {2}, pages = {211216}, url = {http://dx.doi.org/10.1017/S0263034602202086}, doi = {10.1017/S0263034602202086} } 
"Calcium silicate hydrates studied by smallangle neutron scattering (SANS)." Popova A, Geoffroy G, Gartner E and Lapp A, Journal of the American Ceramic Society. Vol. 85(5), pp. 13031305  (2002). 
Abstract: Smallangle neutron scattering (SANS) was used to study calcium silicate hydrate (CSH) formed via pozzolanic reaction between calcium oxide and ultrafine silica in water or polymer solutions at a temperature of 20Â°C. The SANS profile of this product was consistent with a structure that consisted of platelets with maximum diameters of ~ 20 nm (Â± 5 nm) in the xâ€“y plane, which was similar to a structure that had been deduced in previous work via Xray diffractometry. The presence of two different types of superplasticizer in solution (at a concentration of 10 g/L) had no significant effect on its formation kinetics or its SANS profile. 
BibTeX:
@article{Popova2002, author = {Popova, A. and Geoffroy, G. and Gartner, E.M. and Lapp, A.}, title = {Calcium silicate hydrates studied by smallangle neutron scattering (SANS).}, journal = {Journal of the American Ceramic Society}, year = {2002}, volume = {85}, number = {5}, pages = {13031305}, url = {http://onlinelibrary.wiley.com/doi/10.1111/j.11512916.2002.tb00264.x/abstract}, doi = {10.1111/j.11512916.2002.tb00264.x} } 
"A new approach to the thermodynamics of dense plasmas" Blenski T , Pologne (2002). [BibTeX] 
BibTeX:
@inproceedings{InproBlenski22002, author = {Blenski, T.}, title = {A new approach to the thermodynamics of dense plasmas}, year = {2002} } 
"The Radiative Shock : Theory, Laser Experiments and Interpretation" Fleury X, Bouquet S, Koenig M, BenuzziMounaix A, Batani D, Hall T, Grandjouan N, Malka V, Henry E, Leygnac S, Merdji H, Grenier J, Barroso P, Stehlé C, Michaut C, Thais F, Chièze J, Lafon J, Cathala B, Marchet B and Polès L, In Second International Conference on Inertial Fusion Sciences and Applications (IFSA 2001). Kyoto, Japon , pp. 10291033  (2002). 
Abstract: In this paper, a Â« Laser Laboratory Astrophysics Â» study concerning the radiative shock is presented. This kind of shock plays a major role in several astrophysical phenomena (star formation, supernovae explosion, stellar winds ) and the main effects produced by the full radiative contributions (radiative pressure and energy density, in addition to the radiation flux) are reminded from a recent analytical work carried out by us [S. Bouquet, et al., ApJ. Supp. 127, 245 (2000)]. One of the most important effect is the apparition of a radiative precursor. It has been simulated experimentally by using the nanosecond LULI laser. The targets consisted in xenon cells and the physical quantities have been adapted in order to recover the radiative shock conditions. As expected from the theory, the formation and the propagation of a precursor arose. Its velocity and the velocity of the shock have been measured. Comparisons between, on one hand, analytical calculations (selfsimilar solutions) and numerical simulations and, on the other hand, experimental results have been performed and pretty good agreements have been obtained. 
BibTeX:
@inproceedings{InproFleury2002, author = {Fleury, X. and Bouquet, S. and Koenig, M. and BenuzziMounaix, A. and Batani, D. and Hall, T. and Grandjouan, N. and Malka, V. and Henry, E. and Leygnac, S. and Merdji, H. and Grenier, J. and Barroso, P. and Stehlé, C. and Michaut, C. and Thais, F. and Chièze, J.P. and Lafon, J.P. and Cathala, B. and Marchet, B. and Polès, L.}, title = {The Radiative Shock : Theory, Laser Experiments and Interpretation}, booktitle = {Second International Conference on Inertial Fusion Sciences and Applications (IFSA 2001)}, year = {2002}, pages = {10291033} } 
"Rare gas cluster explosion in an intense laser field" Ishikawa K and Blenski T, In 7th Int. Symp. of the Graduate Univ. for Adv. Studies on Science of Superstrong Field Interactions. Shonan Village, Hayama (Japan) Vol. 634(), pp. 211216  (2002). 
Abstract: We study rare gas cluster explosion in an intense, femtosecond laser pulse using Monte Carlo particle dynamics simulations. The obtained dependence of ion energy on ion charge is approximately quadratic for lower charge states and linear for higher ones. This behavior, also observed in experiments, can be entirely explained on the basis of the Coulomb explosion mechanism. Our results also show that electron impact ionization plays only a minor role in ionization. 
BibTeX:
@inproceedings{InproIshikawa2002, author = {Ishikawa, K. and Blenski, T.}, title = {Rare gas cluster explosion in an intense laser field}, booktitle = {7th Int. Symp. of the Graduate Univ. for Adv. Studies on Science of Superstrong Field Interactions}, year = {2002}, volume = {634()}, pages = {211216} } 
"New Radiative Shocks Experiments" Leygnac S, Bouquet S, Stehlé C, BenuzziMounaix A, Boireau L, Chièze JP, Grandjouan N, Huser G, Koenig M, Malka V, Merdji H, Michaut C, Thais F and Vinci T, In Semaine de l'astrophysique franÃ§aise. Paris Vol. (), pp. 531  (2002). 
Abstract: An experimental study of shocks with astrophysical relevance is performedwith the high energy density laser of the LULI, at the école Polytechnique(France). The peculiarity of these shocks is the strong coupling betweenradiation and hydrodynamics which leads to a structure governed by a radiative precursor. A new experiment has been performed this year wherewe have observed shocks identified as radiative shocks. From the measurements, it is possible to infer several features of the shock such as the speed and the electronic density. New diagnostics have been implemented to study the geometrical shape of the shock and obtain spectroscopic informations. 
BibTeX:
@inproceedings{InproLeygnac2002, author = {Leygnac, S. and Bouquet, S. and Stehlé, C. and BenuzziMounaix, A. and Boireau, L. and Chièze, J.P. and Grandjouan, N. and Huser, G. and Koenig, M. and Malka, V. and Merdji, H. and Michaut, C. and Thais, F. and Vinci, T.}, title = {New Radiative Shocks Experiments}, booktitle = {Semaine de l'astrophysique franÃ§aise}, year = {2002}, volume = {()}, pages = {531} } 
"Xray absorption of radiatively heated Al/Ni multilayered foils" Thais F, ChenaisPopovics C, Fajardo M, Gauthier JC, Blenski T, Gilleron F, Pain JC, Poirier M, Eidmann K and Folsner W , In IFSA2001. Japon , pp. 451455  (2002). 
Abstract: Mixtures of light and midZ elements have been used in order to measure the absorption of the midZ element (Ni), the temperature being inferred from the Kshell absorption of the light element (Al). We test here this method by comparing the temperatures deduced from Al Ktransitions and nickel Lshell absorption spectra in Al/Ni bi and multilayers. The temperatures obtained from the experimental spectra using a new version of the opacity code SCO are compared with temperatures predicted by standard hydrodynamic simulations. 
BibTeX:
@inproceedings{InproThais2002, author = {Thais, F. and ChenaisPopovics, C. and Fajardo, M. and Gauthier, J.C. and Blenski, Th. and Gilleron, F. and Pain, J.Ch. and Poirier, M. and Eidmann, K. and Folsner, W.}, title = {Xray absorption of radiatively heated Al/Ni multilayered foils}, booktitle = {IFSA2001}, year = {2002}, pages = {451455} } 
2001 
"Supernovae RayleighTaylor instability experiments on the CEAPhebus laser facility" BenuzziMounaix A, Bouquet S, Chieze JP, Mucchielli F, Teyssier R and Thais F, Astrophysics and Space Science. Vol. 277(12), pp. 143146  (2001). 
Abstract: Hydrodynamic instabilities play a key role in several astrophysical phenomena. We present a laser experiment related to the evolution of RayleighTaylor instabilities (RTI) due to the passage of the shock wave through the He/H interface in a type II supernova. The experiment is performed on the CEAPhébus laser facility and the RTI are studied using a bilayer Cu/CH2 target with sinusoidal ripple at the interface. 
BibTeX:
@article{BenuzziMounaix2001, author = {BenuzziMounaix, A. and Bouquet, S. and Chieze, J.P. and Mucchielli, F. and Teyssier, R. and Thais, F.}, title = {Supernovae RayleighTaylor instability experiments on the CEAPhebus laser facility}, journal = {Astrophysics and Space Science}, year = {2001}, volume = {277}, number = {12}, pages = {143146}, url = {http://link.springer.com/article/10.1023%2FA%3A1012256801365#} doi = {10.1023/A:1012256801365} } 
"Absorption measurements of radiatively heated multilayered Al/Ni foils" ChenaisPopovics C, Fajardo M, Thais F, Gilleron F, Gauthier JC, Eidmann K, Folsner W, Blenski T, Perrot F, BaucheArnoult C, Bachelier A and Bauche J, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 71(26), pp. 249256  (2001). 
Abstract: Mixtures of light and midZ elements have been used to measure the absorption of the midZ element Ni, the temperature is inferred from the Kshell absorption of the light element Al. Here we test this method by comparing the temperatures deduced from Al Ka transitions and nickel Lshell absorption spectra in Al/Ni multilayers and bilayers. The ionisation state is obtained by comparison of the Al and Ni spectra with calculations assuming local thermodynamic equilibrium. The temperatures obtained from the experiment are compared with hydrodynamic simulations predictions. Simulation code results show that the density differs by a factor of 2 in the two elements. This has to be taken into account in the determination of the temperature. 
BibTeX:
@article{ChenaisPopovics2001, author = {ChenaisPopovics, C. and Fajardo, M. and Thais, F. and Gilleron, F. and Gauthier, J.C. and Eidmann, K. and Folsner, W. and Blenski, T. and Perrot, F. and BaucheArnoult, C. and Bachelier, A. and Bauche, J.}, title = {Absorption measurements of radiatively heated multilayered Al/Ni foils}, journal = {Journal of Quantitative Spectroscopy and Radiative Transfer}, year = {2001}, volume = {71}, number = {26}, pages = {249256}, url = {http://www.sciencedirect.com/science/article/pii/S0022407301000723}, doi = {10.1016/S00224073(01)000723} } 
"Rare gas cluster explosion in a strong laser field" Ishikawa K and Blenski T, Laser Physics. Vol. 11(2), pp. 269277  (2001). 
Abstract: We study rare gas cluster explosion in an intense, femtosecond laser pulse using Monte Carlo particle dynamics simulations. The obtained dependence of ion energy on ion charge is approximately quadratic for lower charge states and linear for higher ones. This behavior, also observed in experiments, can be entirely explained on the basis of the Coulomb explosion mechanism. Our results also show that electron impact ionization plays only a minor role in ionization. 
BibTeX:
@article{Ishikawa2001, author = {Ishikawa, K. and Blenski, T.}, title = {Rare gas cluster explosion in a strong laser field}, journal = {Laser Physics}, year = {2001}, volume = {11}, number = {2}, pages = {269277}, url = {http://ishiken.free.fr/Publication/ECLIM2000.pdf} } 
"Series interaction and polarization effects in largeangular momentum twoelectron atoms" Poirier M, Physical Review A. Vol. 63, pp. 052513/114  (2001). 
Abstract: Doubly excited atoms with an outer largel electron are expected to exhibit moderate series interaction. However, accidental or systematic degeneracies may lead to strong configuration mixing. To describe such phenomena, the present formalism uses a partial diagonalization of the dielectronic interaction plus a secondorder correction based on Coulomb Green's function. It makes it possible to determine the eigenfunction composition, level positions, and autoionization widths. While series interaction turns out to be weak for almost degenerate high members of the 4djng series in strontium, a significant configuration mixing is observed on 6pjnl series of barium. A generally fair agreement is observed with 6pjng experimental data. The 6pjnh levels are accurately predicted, too, and new assignations are reported for some of them; however, the computed linewidths are about twice as small as the measured ones. The method also applies to helium and multiply charged ions, where the relevance of collective quantum numbers is analyzed. Some level positions and widths are detailed. 
BibTeX:
@article{Poirier2001, author = {Poirier, M.}, title = {Series interaction and polarization effects in largeangular momentum twoelectron atoms}, journal = {Physical Review A}, year = {2001}, volume = {63}, pages = {052513/114}, url = {http://dx.doi.org/10.1103/PhysRevA.63.052513}, doi = {10.1103/PhysRevA.63.052513} } 
"Absorption d'une feuille d'aluminum à l'équilibre thermodynamique local, pour différentes densités" ChenaisPopovics C, Gilleron F, Thais F, Eidmann K, Folsner W, Gauthier J and Blenski T  (2001). [BibTeX] 
BibTeX:
@techreport{Techreport2001, author = {ChenaisPopovics, C. and Gilleron, F. and Thais, F. and Eidmann, K. and Folsner, W. and Gauthier, J.C. and Blenski, T.}, title = {Absorption d'une feuille d'aluminum à l'équilibre thermodynamique local, pour différentes densités}, year = {2001} } 
2000 
"Radiative heating of B, Al and Ni thin foils at 15  25 eV temperatures" ChenaisPopovics C, Gilleron F, Fajardo M, Merdji H, MiÃŸalla T, Gauthier J, Renaudin P, Gary S, Bruneau J, Perrot F, Blenski T, Folsner W and Eidmann K, Journal of Quantitative Spectroscopy and Radiative Transfer. Vol. 65, pp. 117  (2000). 
Abstract: Several thin foils have been heated by Xray radiation emitted by a small gold cavity irradiated with the LULI facility Nd glass laser. The foils were heated to moderate temperatures (1025 eV) in conditions near local thermodynamic equilibrium. Measurements of the absorption of K transitions of aluminum, of the Kshell transitions of boron, and of the n=23 and 4 transitions of nickel are reported. A 5000 l/mm transmission grating spectrograph recorded the boron data, and a flat thallium hydrogen phthalate (TlAP) crystal was used for aluminum and nickel absorption measurements. The nickel and aluminum spectra indicate a higher temperature (2225 eV) than the boron case (14 eV), explained by a difference in the absorption spectra of these elements. In the Ni case the measured 2p3d spinorbitsplit absorption structures compared well with theoretical spectra obtained with the SCO superconfiguration code using the spin orbit split transition arrays formalism (SOSA). The heating of the foils as calculated with radiative hydrodynamic simulations is very similar to the experimental data. 
BibTeX:
@article{ChenaisPopovics2000a, author = {ChenaisPopovics, C. and Gilleron, F. and Fajardo, M. and Merdji, H. and Mißalla, T. and Gauthier, J.C. and Renaudin, P. and Gary, S. and Bruneau, J. and Perrot, F. and Blenski, T. and Folsner, W. and Eidmann, K.}, title = {Radiative heating of B, Al and Ni thin foils at 15  25 eV temperatures}, journal = {Journal of Quantitative Spectroscopy and Radiative Transfer}, year = {2000}, volume = {65}, pages = {117}, url = {http://dx.doi.org/10.1016/S00224073(99)000618}, doi = {10.1016/S00224073(99)000618} } 
"Opacity studies of iron in the 1530eV temperature range" ChenaisPopovics C, Merdji H, MiÃŸalla T, Gilleron F, Gauthier JC, Blenski T, Perrot F, Klapisch M, BaucheArnoult C, Bauche J, Bachelier A and Eidmann K, Astrophysical Journal. Supplement series. Vol. 127(2), pp. 275281  (2000). 
Abstract: Absorption of the 2p3d transitions of iron has been measured using point projection spectroscopy. Thin C tamped Fe foils were heated around 20 eV by Xrays generated in gold spherical hohlraums irradiated by the highpower laser ASTERIX IV. Absorption of Fe V to Fe X has been observed in the spectral vicinity of 730 eV (17 Ä¹). The Ag backlighter source and absorbed spectra were recorded on the same shot by a TlAP crystal spectrograph. The experimental spectra have been reproduced by the two superconfiguration local thermodynamic equilibrium codes SCO and STA. Detailed statistical calculations of the different ionic structures have also been performed with the Spin Orbit Split Arrays method, allowing the determination of ion populations. The electron temperature and average ionization obtained by fitting the experiment with the different calculations were compared with radiative hydrodynamic simulations. 
BibTeX:
@article{ChenaisPopovics2000, author = {ChenaisPopovics, C. and Merdji, H. and MiÃŸalla, T. and Gilleron, F. and Gauthier, J. C. and Blenski, T. and Perrot, F. and Klapisch, M. and BaucheArnoult, C. and Bauche, J. and Bachelier, A. and Eidmann, K.}, title = {Opacity studies of iron in the 1530eV temperature range}, journal = {Astrophysical Journal. Supplement series}, year = {2000}, volume = {127}, number = {2}, pages = {275281}, url = {http://dx.doi.org/10.1086/313354} } 
"Explosion dynamics of rare gas clusters in an intense laser field" Ishikawa K and Blenski T, Physical Review A. Vol. 62(6), pp. 063204/111  (2000). 
Abstract: We study the explosion dynamics of raregas clusters (Ar55, Ar147, Xe55, and Xe147) in an intense, femtosecond laser pulse via Monte Carlo classical particledynamics simulations. Our method includes tunnel and impact ionization as well as ionelectron recombination, and allows us to follow the motion of both ions and free electrons during lasercluster interaction. Our simulation results show that ionization proceeds mainly through tunnel ionization by the combined fields from ions, electrons, and laser while the contribution of electronimpact ionization is secondary. The ions are ejected in a stepwise manner from outer shells and accelerated mainly through their mutual Coulomb repulsion. Taking a spatial laser intensity profile into account, we show that the Coulomb explosion scenario leads to the same charge dependence of ion energy, i.e., quadratic for lower charge states and linear for higher ones, as that observed in experiments with larger clusters. This indicates that Coulomb explosion may be a dominant cluster explosion mechanism even in the case of large clusters. We also find that the ion energy is higher in the direction parallel to laser polarization than in the direction perpendicular to it. When ions are emitted along the direction of laser polarization, their charge changes in phase with the laser field, and this leads to an efficient acceleration. 
BibTeX:
@article{Ishikawa2000, author = {Ishikawa, K. and Blenski, T.}, title = {Explosion dynamics of rare gas clusters in an intense laser field}, journal = {Physical Review A}, year = {2000}, volume = {62}, number = {6}, pages = {063204/111}, url = {http://dx.doi.org/10.1103/PhysRevA.62.063204}, doi = {0.1103/PhysRevA} } 
"Simulations "Particleincell" d'ionisations multiples de petites molécules dans un champ de laser intense.Particleincell simulations of multiple ionization of small molecules in a strong laser field." Ishikawa K and Blenski T, Physical Review A. Vol. 61, pp. 063408  (2000). 
Abstract: Nous présentons des simulations "Particleincell" (PIC) à une dimension appliquées à l'ionisation multiple et à la fragmentation de molécules di et triatomiques soumises à un cham laser intense ultracourt. Notre méthode permet de traiter tous les électrons et tous les noyaux explicitement et de suivre l'évolution temporaire de l'ionisation. Les résultats des simulations confirment que la probabilité d'ionisation est fortement augmentée à une certaine distance critique internucléaire (enhanced ionization). Ce phénomène a lieu quand les barrières internes du potentiel sont plus hautes que celle externe. Le mécanisme de "enhanced ionization" dans une molécule triatomique se comprend de manière similaire au cas diatomique, bien que les trois puits de potentiel y participent dans le cas triatomique. Malgré le phénomène, l'ionization n'est pas nécessairement localisée à la distance critique. D'ailleurs nos simulations montrent qu'il n'y a pas de différences significatives en ce qui concerne l'état de charge des fragments ioniques entre le cas des molécules di et triatomique. La faible valeur de la distance critique dans nos résultats peut impliquer que le défaut de l'énergie cinétique observé expérimentalement soit causé non seulement par "enhanced ionization" autour de cette distance mais aussi par la nature noncouloumbienne du potentiel moléculaire. 
BibTeX:
@article{Ishikawa2000a, author = {Ishikawa, K. and Blenski, T.J.}, title = {Simulations "Particleincell" d'ionisations multiples de petites molécules dans un champ de laser intense.Particleincell simulations of multiple ionization of small molecules in a strong laser field.}, journal = {Physical Review A}, year = {2000}, volume = {61}, pages = {063408}, url = {http://dx.doi.org/10.1103/PhysRevA.61.063408}, doi = {0.1103/PhysRevA.61.063408} } 
"SANS study of the microstructural evolution of martensitic steels under thermal ageing and neutron irradiation." Mathon M, Geoffroy G, De Carlan Y, Alamo A and De novion C, Physica B. Vol. 27677, pp. 939940  (2000). 
Abstract: SANS technique has been used to study the microstructural evolution of martensitic steels containing 712% Cr, under thermal ageing and neutron irradiation. Some of the investigated alloys are industrial low activation martensitic (LAM) materials, where alloying elements have been substituted by elements with low radiological impact. For materials quenched from the austenitic phase, a direct correlation was found between the hardening and the number density of M2C precipitates induced by thermal ageing at 500 Â°C. Irradiationaccelerated spinodal decomposition of the B.C.C. ferrite was observed in alloys containing large (= 11%) chromium content. 
BibTeX:
@article{Mathon2000, author = {Mathon, M. and Geoffroy, G. and De Carlan, Y. and Alamo, A. and De novion, C.}, title = {SANS study of the microstructural evolution of martensitic steels under thermal ageing and neutron irradiation.}, journal = {Physica B}, year = {2000}, volume = {27677}, pages = {939940}, url = {http://hal.archivesouvertes.fr/hal00725142/}, doi = {10.1016/S09214526(99)012995} } 
"Absorption X de feuilles multicouches d'aluminiumnickel chauffées radiativement" ChenaisPopovics C, Fajardo M, Gilleron F, Gauthier JC, Thais F, Folsner W, Eidmann K, Perrot F and Blenski T  (2000). [BibTeX] 
BibTeX:
@techreport{Techreport2000, author = {ChenaisPopovics, C. and Fajardo, M. and Gilleron, F. and Gauthier, J.C. and Thais, F. and Folsner, W. and Eidmann, K. and Perrot, F. and Blenski, T.}, title = {Absorption X de feuilles multicouches d'aluminiumnickel chauffées radiativement}, year = {2000} } 
"Absorption of Xrays in dense plasmas" Blenski T, Pologne  (2000). [BibTeX] 
BibTeX:
@inproceedings{InproBlenski32000, author = {Blenski, T.}, title = {Absorption of Xrays in dense plasmas}, year = {2000} } 
"XRay Absorption In Dense Plasmas Theory vs. Experiment" Blenski T, Perrot F, Renaudin P, ChenaisPopovics C, Fajardo M, Merdji H, Gilleron F, Gauthier JC, Eidmann K and Andiel U, In IFSA1999. France , pp. 11111114  (2000). [BibTeX] 
BibTeX:
@inproceedings{0InproBlenski22000, author = {Blenski, T. and Perrot, F. and Renaudin, P. and ChenaisPopovics, C. and Fajardo, M. and Merdji, H. and Gilleron, F. and Gauthier, JC. and Eidmann, K. and Andiel, U.}, title = {XRay Absorption In Dense Plasmas Theory vs. Experiment}, booktitle = {IFSA1999}, year = {2000}, pages = {11111114} } 
"The Astrolab experiment : RayleighTaylor instabilities in supernova" Thais F, Chièze J, Baclet P, Benuzzi A, Bouquet S, Cherfils C, Mucchielli F, Polès L, Reverdin C, Teyssier R, Thébault J and Troussel P, In IFSA 1999. Bordeaux (France) Vol. (), pp. 10831086  (2000). 
Abstract: Hydrodynamic instabilities play a key role in several astrophysical phenomena. Here we present a laser experiment related to the evolution of RayleighTaylor instabilities at the passage of the shock wave through the He/H interface in a type II supernova. The growth rate of the instabilities is studied for different initial conditions using a bilayer Cu/CH2 target with sinusoidal ripple at the interface. The experiment is performed on the PHéBUS laser facility, in an indirect drive configuration. 
BibTeX:
@inproceedings{InproThais2000, author = {Thais, F. and Chièze, J.P. and Baclet, P. and Benuzzi, A. and Bouquet, S. and Cherfils, C. and Mucchielli, F. and Polès, L. and Reverdin, C. and Teyssier, R. and Thébault, J.P. and Troussel, P.}, title = {The Astrolab experiment : RayleighTaylor instabilities in supernova}, booktitle = {IFSA 1999}, year = {2000}, volume = {()}, pages = {10831086} } 
1999 
"Observation of ions with energies above 100 keV produced by the interaction of a 60fs laser pulse with clusters" Dobosz S, Schmidt M, Perdrix M, Meynadier P, Gobert O, Normand D, Ellert C, Blenski T, Faenov AY, Magunov IA, Pikuz T, Skobelev IY and Andreev NE, Journal of Experimental and Theoretical Physics. Vol. 88(6), pp. 11221129  (1999). 
Abstract: The xray spectra of a plasma generated by heating CO2 and Ar clusters with highintensity femtosecond laser pulses with qlas ~ 1018 W/cm2 are investigated. Spatially resolved xray spectra of a cluster plasma are obtained for the first time. Photoionization absorption is observed to influence the spectral line profiles. The recorded features of the xray emission spectra definitely indicate the existence of a large relative number of excited ions (=~102â€“103) with energies of 0.1â€“1 MeV in such a plasma. Possible mechanisms underlying the acceleration of ions to high energies are discussed. It is shown that the experimental results can be attributed to the influence of ponderomotive forces in standing waves generated by the reflection of laser radiation from the clusters. 
BibTeX:
@article{Dobosz1999, author = {Dobosz, S. and Schmidt, M. and Perdrix, M. and Meynadier, P. and Gobert, O. and Normand, D. and Ellert, C. and Blenski, T. and Faenov, A. Ya. and Magunov, I. A. and Pikuz, T.A. and Skobelev, I. Yu. and Andreev, N. E.}, title = {Observation of ions with energies above 100 keV produced by the interaction of a 60fs laser pulse with clusters}, journal = {Journal of Experimental and Theoretical Physics}, year = {1999}, volume = {88}, number = {6}, pages = {11221129}, url = {http://dx.doi.org/10.1134/1.558900}, doi = {10.1134/1.558900} } 
"Effets de polarisation lors des processus d'autoionisation des atomes alcalinoterreux : analyse par la fonction de Green Coulombienne.Polarization effects in autoionisation processes of alkalineearth atoms : Coulomb Green's function analysis." Poirier M and Semaoune R, Physical Review A. Vol. 59(5), pp. 34713479  (1999). 
Abstract: Dans les systèmes multiélectroniques, la corrélation électronique qui est la manifestation du comportement nonindépendant des électrons joue un rôle important à plus d'un titre : la classification des états doublement excités doit la prendre en compte, les positions de ces mêmes états en dépendent fortement et, récemment divers travaux ont souligné le lien entre l'apparition du chaos et la présence des corrélations. A priori les atomes doublement excités de grand moment cinétique, dans lesquels l'orbitale de l'électron le plus excité (de grand moment l) ne recouvre pratiquement pas celle de l'électron moins excité ni le coeur atomique, ne sont pas les candidats idéaux pour étudier de tels effets ; une description par la théorie de perturbations à l'ordre le plus bas qui ignore les corrélations devrait alors suffire. Or un précédent travail portant sur les premiers états doublement excités de grand l des alcalinoterreux (3dng du calcium, 4dng du strontium, 5dng du baryum, donc avec l égal à 4) a établi que leurs positions sont décrites de manière très insuffisante par la théorie des perturbations à l'ordre le plus bas. Il en est de même pour le calcul des probabilités d'autoionisation, processus caractéristique des états doublement excités et principalement responsable de la largeur de ces états. Le présent travail, en développant le calcul en perturbation jusqu'à l'ordre 2 à l'aide de la technique de la fonction de Green Coulombienne, permet d'obtenir pour les largeurs des états 5d5g du baryum un accord tout à fait satisfaisant avec les données expérimentales existantes. Cette description théorique correspond physiquement à la prise en compte de la polarisation (déformation à distance) de l'orbitale de l'électron interne par l'électron externe. Plus généralement, il est montré ici que ce phénomène se manifeste sur chacun des états doublement excités des alcalinoterreux mentionnés plus haut. A la différence des positions de niveaux qui peuvent être comparées à un vaste ensemble de données expérimentales, les largeurs calculées ici constituent dans leur grande majorité des déterminations originales et leur confirmation expérimentale est vivement souhaitée. Toutefois, dans le cas des niveaux 5d5/2nh J=5 du baryum, pour lesquels la description théorique devrait à fortiori être pertinente puisque le moment l est encore plus grand (5 au lieu de 4), l'accord avec une mesure réalisée à l'Université d'Amsterdam s'avère excellent. 
BibTeX:
@article{Poirier1999, author = {Poirier, M. and Semaoune, R.}, title = {Effets de polarisation lors des processus d'autoionisation des atomes alcalinoterreux : analyse par la fonction de Green Coulombienne.Polarization effects in autoionisation processes of alkalineearth atoms : Coulomb Green's function analysis.}, journal = {Physical Review A}, year = {1999}, volume = {59}, number = {5}, pages = {34713479}, url = {http://prola.aps.org/abstract/PRA/v59/i5/p3471_1}, doi = {10.1103/PhysRevA.59.3471} } 