High-Precision Equation-of-State Formalisms for Solar and Stellar Modeling

被引：1
|
作者：
Daeppen, Werner [1 ]
机构：
[1] Univ So Calif, Dept Phys & Astron, Los Angeles, CA 90089 USA
来源：
CONTRIBUTIONS TO PLASMA PHYSICS | 2011年 / 51卷 / 04期
基金：
美国国家科学基金会;
关键词：
Equation of state; Stars: evolution; Sun: helioseismology; CHEMICAL-COMPOSITION; VIRIAL EXPANSIONS; QUANTUM PLASMAS; THERMODYNAMIC FUNCTIONS; SUN; HELIOSEISMOLOGY; ENVELOPES; INTERIOR; ABUNDANCE; SEISMOLOGY;
D O I：
10.1002/ctpp.201010121
中图分类号：
O35 [流体力学]; O53 [等离子体物理学];
学科分类号：
070204 ; 080103 ; 080704 ;
摘要：
For solar and stellar modeling, a high-quality equation of state is crucial. In addition, however, helioseismic and asteroseismic observations put constraints on the physical formalisms. Thus they effectively turn the Sun and the stars into laboratories for dense plasmas. Currently, the main astrophysical beneficiary of a good equation of state is the seismic determination of the chemical composition of the interior of the Sun and stars. (C) 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
引用
收藏
页码：328 / 332
页数：5
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