activity
20092020
most citedReview of the First Charged-Particle Transport Coefficient Comparison Workshop

87 citations · 222 across the 8 of their papers we have counts for

collaborators

8 papers

physics.plasm-ph2020★ 87 cited

Review of the First Charged-Particle Transport Coefficient Comparison Workshop

P. E. Grabowski, S. B. Hansen, M. S. Murillo +42

We present the results of the first Charged-Particle Transport Coefficient Code Comparison Workshop, which was held in Albuquerque, NM October 4-6, 2016. In this first workshop, sc…

physics.atom-ph2016★ 24 cited

Comment on "Large enhancement in high-energy photoionization of Fe XVII and missing continuum plasma opacity"

C. Blancard, J. Colgan, Ph. Cossé +12

Recent R-matrix calculations claim to produce a significant enhancement in the opacity of Fe XVII due to atomic core excitations [S. N. Nahar & A.K. Pradhan, Phys. Rev. Letters 116…

astro-ph.SR2015★ 29 cited

First solar models with OPAS opacity tables

Maëlle Le Pennec, Sylvaine Turck-Chièze, Sébastien Salmon +4

Stellar seismology appears more and more as a powerful tool for a better determination of the fundamental properties of solar-type stars. However the particular case of Sun is stil…

astro-ph.SR2012★ 32 cited

Comparison of Fe and Ni opacity calculations for a better understanding of pulsating stellar envelopes

D. Gilles, S. Turck-Chièze, G. Loisel +19

Opacity is an important ingredient of the evolution of stars. The calculation of opacity coefficients is complicated by the fact that the plasma contains partially ionized heavy io…

astro-ph.SR2012★ 2 cited

Iron and Nickel spectral opacity calculations in conditions relevant for pulsating stellar envelopes and experiments

D. Gilles, S. Turck-Chièze, M. Busquet +18

Seismology of stars is strongly developing. To address this question we have formed an international collaboration OPAC to perform specific experimental measurements, compare opaci…

astro-ph.SR2011★ 15 cited

Theoretical and experimental activities on opacities for a good interpretation of seismic stellar probes

S Turck-Chièze, G Loisel, D Gilles +23

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…

astro-ph.SR2011★ 17 cited

Radiative properties of stellar plasmas and open challenges

S. Turck-Chièze, G. Loisel, D. Gilles +24

The lifetime of solar-like stars, the envelope structure of more massive stars, and stellar acoustic frequencies largely depend on the radiative properties of the stellar plasma. U…

physics.atom-ph2009★ 16 cited

Jensen-Feynman approach to the statistics of interacting electrons

Jean-Christophe Pain, Franck Gilleron, Gerald Faussurier

Faussurier et al. [Phys. Rev. E 65, 016403 (2001)] proposed to use a variational principle relying on Jensen-Feynman (or Gibbs-Bogoliubov) inequality in order to optimize the accou…