학술논문
Theoretical and experimental activities on opacities for a good interpretation of seismic stellar probes
Document Type
Working Paper
Author
Turck-Chièze, S; Loisel, G; Gilles, D; Thais, F; Bastiani, S; Blancard, C; Busquet, M; Caillaud, T; Cosse, P; Blenski, T; Delahaye, F; Ducret, J E; Faussurier, G; Gilleron, F; Guzik, J; Harris, J W; Kilcrease, D P; Magee, N H; Piau, L; Pain, J C; Poirier, M; Porcherot, Q; Reverdin, C; Silvert, V; Villette, B; Zeippen, C
Source
Journal of Physics: conf series 2011
Subject
Language
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.
Comment: 6 pages, 4 figures, invited talk at SOHO24
Comment: 6 pages, 4 figures, invited talk at SOHO24