Phys. Rev. Lett. 26, 1344–1346 (1971)Gravitational Radiation from Colliding Black HolesReceived 11 March 1971; published in the issue dated 24 May 1971 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. © 1971 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevLett.26.1344
DOI:
10.1103/PhysRevLett.26.1344
PACS:
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