Formation of black holes in general relativity
In 1965 Penrose introduced the fundamental concept of a trapped surface, on the basis of which he proved a theorem which asserts that a spacetime containing such a surface must come to an end. The presence of a trapped surface implies, moreover, that there is a region of spacetime, the black hole, w...
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Format: | Book |
Language: | English |
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[Place of publication not identified] :
EUROPEAN MATHEMATICAL SOCIETY,
2009
[Place of publication not identified] : EUROPEAN MATHEMATICAL Society, 2009 |
Series: | EMS monographs in mathematics
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Internet
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ISIL:US-CST |
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