Gravitational Radiation from Colliding Black Holes

Details Gravitational Radiation from Colliding Black Holes Gravitational Radiation from Colliding Black Holes

May 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971phrvl..26.1344h&link_type=abstract

Physical Review Letters, vol. 26, Issue 21, pp. 1344-1346

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271

Scientific paper

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 (2-2)m.

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