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

Journal Article:

Abstract

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.
Authors:
Miller, J C [1] 
  1. Oxford Univ. (UK). Dept. of Astrophysics
Publication Date:
May 01, 1977
Product Type:
Journal Article
Reference Number:
AIX-08-326705; EDB-77-149590
Resource Relation:
Journal Name: Mon. Not. R. Astron. Soc.; (United Kingdom); Journal Volume: 179:2
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; GRAVITATIONAL COLLAPSE; GENERAL RELATIVITY THEORY; STARS; ANGULAR VELOCITY; BLACK HOLES; ROTATION; STAR MODELS; FIELD THEORIES; MATHEMATICAL MODELS; MOTION; VELOCITY; 657003* - Theoretical & Mathematical Physics- Relativity & Gravitation; 640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
7213833
Country of Origin:
United Kingdom
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: MNRAA
Submitting Site:
INIS
Size:
Pages: 483-498
Announcement Date:
Oct 01, 1977

Journal Article:

Citation Formats

Miller, J C. Quasi-stationary gravitational collapse of slowly rotating bodies in general relativity. United Kingdom: N. p., 1977. Web.
Miller, J C. Quasi-stationary gravitational collapse of slowly rotating bodies in general relativity. United Kingdom.
Miller, J C. 1977. "Quasi-stationary gravitational collapse of slowly rotating bodies in general relativity." United Kingdom.
@misc{etde_7213833,
title = {Quasi-stationary gravitational collapse of slowly rotating bodies in general relativity}
author = {Miller, J C}
abstractNote = {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.}
journal = {Mon. Not. R. Astron. Soc.; (United Kingdom)}
volume = {179:2}
journal type = {AC}
place = {United Kingdom}
year = {1977}
month = {May}
}