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  Final spin from the coalescence of two black holes

Rezzolla, L., Barausse, E., Dorband, E. N., Pollney, D., Reisswig, C., Seiler, J., et al. (2008). Final spin from the coalescence of two black holes. Physical Review D, 78(4): 044002. doi:10.1103/PhysRevD.78.044002.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-13B9-3 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-002C-4BB9-C
Genre: Journal Article

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PRD78-044002.pdf (Publisher version), 206KB
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 Creators:
Rezzolla, Luciano1, Author              
Barausse, Enrico2, Author
Dorband, Ernst Nils1, Author              
Pollney, Denis1, Author              
Reisswig, Christian1, Author              
Seiler, Jennifer1, Author              
Husa, Sascha1, Author              
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1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              
2External Organizations, ou_persistent22              

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 Abstract: We provide a compact analytic formula to compute the spin of the black hole produced by the coalescence of two black holes following a quasicircular inspiral. Without additional fits than those already available for binaries with aligned or antialigned spins, but with a minimal set of assumptions, we derive an expression that can model generic initial spin configurations and mass ratios, thus covering all of the 7-dimensional space of parameters. A comparison with simulations already shows very accurate agreements with all of the numerical data available to date, but we also suggest a number of ways in which our predictions can be further improved.

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 Dates: 2008-08-01
 Publication Status: Published online
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 Rev. Method: Peer
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Title: Physical Review D
Source Genre: Journal
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Pages: - Volume / Issue: 78 (4) Sequence Number: 044002 Start / End Page: - Identifier: ISSN: 1089-4918