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Issue 12, 2025
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Reviews of topical problems


Relativistic astrophysics. I

 a,  b, c, d
a Russian Federal Nuclear Center - All-Russian Research Institute of Experimental Physics, prosp. Mira 37, Sarov, Nizhny Novgorod region, 607188, Russian Federation
b National Research Centre ‘Kurchatov Institute’, pl. akad. Kurchatova 1, Moscow, 123182, Russian Federation
c Astro Space Centre, Lebedev Physical Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, Moscow, 117997, Russian Federation
d Niels Bohr Institute, Blegdamsvej 17, Copenhagen, DK-2100, Denmark

CONTENTS
1. Introduction 763
2. Equilibrium and Stability of a Star as a Whole 764
3. Equation of State 767
4. Masses of Stars in the Final Stages of Evolution 769
5. Schwarzschild Gravitation Field 770
6. Gravitational Field Inside a Star 771
7. Paths of Light Rays Inside and Outside a Static Star 772
8. Structure of Superdense Stars 773
9. Mass Defect 775
10. Stability of Superdense Stars 776
11. Solutions with Negative Gravitational Mass Defect 777
12. Evolution of a Star 778
13. Neutron Stars 781
14. Evolution of a Star with a Mass Larger than the "OV" Limit 782
15. Relativistic Collapse 783
16. Metastability of any Equilibrium State 786
Cited literature 787

Fulltext pdf (2.4 MB)
Fulltext is also available at DOI: 10.1070/PU1965v007n06ABEH003683
PACS: 95.30.Tg, 97.10.Nf, 97.60.Jd, 97.10.Cv, 95.30.Sf (all)
DOI: 10.1070/PU1965v007n06ABEH003683
URL: https://ufn.ru/en/articles/1965/6/a/
Citation: Zel’dovich Ya B, Novikov I D "Relativistic astrophysics. I" Sov. Phys. Usp. 7 763–788 (1965)
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Îðèãèíàë: Çåëüäîâè÷ ß Á, Íîâèêîâ È Ä «Ðåëÿòèâèñòñêàÿ àñòðîôèçèêà. I» ÓÔÍ 84 377–417 (1964); DOI: 10.3367/UFNr.0084.196411a.0377

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