3D grazing collision of two black holes

Miguel Alcubierre, Werner Benger, Bernd Brügmann, Gerd Lanfermann, Lars Nerger, Edward Seidel, Ryoji Takahashi

Research output: Contribution to journalArticle

Abstract

The results for two colliding black holes (BH) with angular momentum, spin and unequal mass were presented. A full 3D numerical evolution was used for the computation of gravitational waveforms for a grazing collision. It was shown that the total energy radiated in gravitational waves was consistent with the total initial mass of the spacetime and the apparent horizon mass of the final BH.

Original languageEnglish (US)
Article number271103
Pages (from-to)2711031-2711034
Number of pages4
JournalPhysical review letters
Volume87
Issue number27 I
StatePublished - Dec 31 2001
Externally publishedYes

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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