Relativistic effects in the solar EOS -: A helioseismic forward analysis

被引:4
|
作者
Bonanno, A
Murabito, AL
Paternò, L
机构
[1] Osserv Astrofis Catania, I-95123 Catania, Italy
[2] Univ Catania, Dipartimento Fis & Astron, Sez Astrofis, I-95123 Catania, Italy
来源
ASTRONOMY & ASTROPHYSICS | 2001年 / 375卷 / 03期
关键词
Sun : interior; Sun : oscillations; equation of state;
D O I
10.1051/0004-6361:20010946
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the sensitivity of the sound speed to relativistic corrections of the equation of state (EOS) in the standard solar model by means of a helioseismic forward analysis. We use the latest GOLF/SOHO data for l = 0, 1, 2, 3 modes to confirm that the inclusion of the relativistic corrections to the adiabatic exponent Gamma (1) computed from both OPAL and MHD EOS leads to a more reliable theoretical modelling of the innermost layers of the Sun.
引用
收藏
页码:1062 / 1064
页数:3
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