Title: Gravitational Radiation from Colliding Black Holes
Abstract: It is shown that there is an upper bound to the energy of the gravitational radiation emitted when one collapsed object captures another. In the case of two objects with equal masses $m$ and zero intrinsic angular momenta, this upper bound is $(2\ensuremath{-}\sqrt{2})m$.
Publication Year: 1971
Publication Date: 1971-05-24
Language: en
Type: article
Indexed In: ['crossref']
Access and Citation
Cited By Count: 975
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