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Trapped surfaces in spherical stars
The conditions under which a spherically symmetric star will collapse to a black hole are considered analytically, with a focus on the local property known as a trapped surface, defined as a closed two-surface from which, at any instant of time, outgoing light rays are convergent. Necessary and suff...
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Published in: | Physical review letters 1988-09, Vol.61 (10), p.1147-1150 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The conditions under which a spherically symmetric star will collapse to a black hole are considered analytically, with a focus on the local property known as a trapped surface, defined as a closed two-surface from which, at any instant of time, outgoing light rays are convergent. Necessary and sufficient conditions for the existence of trapped surfaces in spherically symmetric space-times are derived, and their implications for the cosmic- censorship hypothesis are explored. It is shown that both the degree of concentration and the average matter flow determine whether trapped surfaces can form. (T.K.) |
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ISSN: | 0031-9007 1079-7114 |
DOI: | 10.1103/PhysRevLett.61.1147 |