Quasi-stationary gravitational collapse of slowly rotating bodies in general relativity

Details Quasi-stationary gravitational collapse of slowly rotating bodies in general relativity Quasi-stationary gravitational collapse of slowly rotating bodies in general relativity

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.179..483m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 179, May 1977, p. 483-498. Research supported by the Science Research C

Astronomy and Astrophysics

Astronomy

21

Black Holes (Astronomy), Gravitational Collapse, Relativity, Rotating Bodies, Stellar Models, Astronomical Models, Dynamic Characteristics, Ellipticity, Isobars, Quasi-Steady States, Schwarzschild Metric, Stellar Evolution

Scientific paper

This paper presents results of quasi-stationary collapse calculations for a class of slowly rotating non-homogeneous bodies in general relativity. The results are qualitatively similar to those obtained previously for homogeneous models indicating that the effects described for the homogeneous models are likely to have some relevance for the gravitational collapse of real stars towards the black hole state. There is also a discussion of some basic questions associated with such calculations.

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