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Energy and angular momentum radiated for non head-on binary black hole collisions

Osvaldo Moreschi·Alejandro Perez·Luis Lehner
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Abstract

We investigate the possible total radiated energy produced by a binary black hole system containing non-vanishing total angular momentum. For the scenearios considered we find that the total radiated energy does not exceed 1%. Additionally we explore the gravitational radiation field and the variation of angular momentum in the process.

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Osvaldo Moreschi, Alejandro Perez, Luis Lehner. 2002-09-17. Energy and angular momentum radiated for non head-on binary black hole collisions. https://doi.org/10.1103/physrevd.66.104017

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