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Issue 4, 2024
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Reviews of topical problems


Relativistic astrophysics. II

 a,  b, c, d
a All-Russian Scientific Research Institute of Experimental Physics — Federal Nuclear Centre, prosp. Mira 37, Sarov, Nizhny Novgorod region, 607190, 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 522
2. Equilibrium of Supermassive Star 524
3. Equilibrium of Rotating Star with γ = 4/3 529
4. The Possible Occurrence of a Supermassive Star 531
5. Evolution of Supermassive Star 532
6. Evolution of Star of Medium Mass 537
7. Motion of Trial Particles and Light Rays in a Schwarzschild Field 544
8. Radiation of Gravitational Waves 547
9. Collapse of Rotating Star 549
10. Collapse of Nonspherical Body 551
11. Does Rapid Rotation Interfere with Collapse of a Star? 552
12. Comparison with Observations 553
13. Accretion of Gas by Neutron and Cooled Stars 557
14. Magnetic and Magnetohydrodynamic Phenomena 563
15. Quasars ("Superstars") 567
16. Magnetoturbulent Theory of Quasars 568
17. The Anticollapse Hypothesis 570
Appendix 571
Cited Literature 574

PACS: 97.10.Kc, 97.10.Cv, 97.10.Gz, 97.60.Jd, 95.30.Qd, 98.54.Aj (all)
DOI: 10.1070/PU1966v008n04ABEH002990
URL: https://ufn.ru/en/articles/1966/4/c/
Citation: Zel’dovich Ya B, Novikov I D "Relativistic astrophysics. II" Sov. Phys. Usp. 8 522–577 (1966)
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Îðèãèíàë: Çåëüäîâè÷ ß Á, Íîâèêîâ È Ä «Ðåëÿòèâèñòñêàÿ àñòðîôèçèêà. II» ÓÔÍ 86 447–536 (1965); DOI: 10.3367/UFNr.0086.196507f.0447

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