Solar structure and evolution

被引：64

作者：

Christensen-Dalsgaard, Jorgen ^{[1
,2
]}

机构：

[1] Aarhus Univ, Stellar Astrophys Ctr, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

[2] Aarhus Univ, Dept Phys & Astron, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

来源：

LIVING REVIEWS IN SOLAR PHYSICS | 2021年 / 18卷 / 01期

基金：

新加坡国家研究基金会;

关键词：

Stellar structures; Stellar evolution; Solar evolution; Solar interior; EQUATION-OF-STATE; ANGULAR-MOMENTUM TRANSPORT; 3D CONVECTION SIMULATIONS; STELLAR STRUCTURE MODELS; INTERNAL GRAVITY-WAVES; PRE-MAIN-SEQUENCE; INTERACTING MASSIVE PARTICLES; FREQUENCY-SEPARATION RATIOS; OXYGEN ISOTOPIC COMPOSITION; OSCILLATION NETWORK GROUP;

D O I：

10.1007/s41116-020-00028-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Sun provides a critical benchmark for the general study of stellar structure and evolution. Also, knowledge about the internal properties of the Sun is important for the understanding of solar atmospheric phenomena, including the solar magnetic cycle. Here I provide a brief overview of the theory of stellar structure and evolution, including the physical processes and parameters that are involved. This is followed by a discussion of solar evolution, extending from the birth to the latest stages. As a background for the interpretation of observations related to the solar interior I provide a rather extensive analysis of the sensitivity of solar models to the assumptions underlying their calculation. I then discuss the detailed information about the solar interior that has become available through helioseismic investigations and the detection of solar neutrinos, with further constraints provided by the observed abundances of the lightest elements. Revisions in the determination of the solar surface abundances have led to increased discrepancies, discussed in some detail, between the observational inferences and solar models. I finally briefly address the relation of the Sun to other similar stars and the prospects for asteroseismic investigations of stellar structure and evolution.

引用

页数：189

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