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  Inspiralling Black holes: The close limit

Khanna, G., Baker, J. G., Gleiser, R. J., Laguna, P., Nicasio, C. O., Nollert, H.-P., et al. (1999). Inspiralling Black holes: The close limit. Physical Review Letters, 83(18), 3581-3584. doi:10.1103/PhysRevLett.83.3581.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-58BA-A Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-58BB-8
Genre: Journal Article

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PRL83-18-1999.pdf (Publisher version), 60KB
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 Creators:
Khanna, Gaurav, Author
Baker, John G.1, Author
Gleiser, Reinaldo J., Author
Laguna, Pablo, Author
Nicasio, Carlos O., Author
Nollert, Hans-Peter, Author
Price, Richard, Author
Pullin, Jorge, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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 Abstract: We calculate an estimate of the gravitational radiation emitted when two equal mass black holes coalesce at the end of their binary inspiral, using several approximations based on considering the holes close to each other. A shortcoming of our method is that it is limited to models forming final holes with slow rotation, but our results clearly suggest a trend for larger angular momenta. We find that about 1% of the mass energy of the pair will emerge as gravitational waves during the final stages of the collision and that a negligible fraction of the angular momentum will be radiated.

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 Dates: 1999
 Publication Status: Published in print
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Title: Physical Review Letters
Source Genre: Journal
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Pages: - Volume / Issue: 83 (18) Sequence Number: - Start / End Page: 3581 - 3584 Identifier: ISSN: 1079-7114