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  Accurate Evolutions of Orbiting Binary Black Holes

Diener, P., Herrmann, F., Pollney, D., Schnetter, E., Seidel, E., Takahashi, R., et al. (2006). Accurate Evolutions of Orbiting Binary Black Holes. Physical Review Letters, 171-174.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4BA7-C Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4BA8-A
Genre: Conference Paper

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249144.pdf (Publisher version), 256KB
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 Creators:
Diener, Peter, Author
Herrmann, Frank1, Author
Pollney, Denis1, Author              
Schnetter, Erik1, Author
Seidel, Edward1, Author
Takahashi, Ryoji, Author
Thornburg, Jonathan1, Author
Ventrella, Jason, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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 Abstract: We present a detailed analysis of binary black hole evolutions in the last orbit and demonstrate consistent and convergent results for the trajectories of the individual bodies. The gauge choice can significantly affect the overall accuracy of the evolution. It is possible to reconcile certain gauge-dependent discrepancies by examining the convergence limit. We illustrate these results using an initial data set recently evolved by Brügmann et al. [Phys. Rev. Lett. 92, 211101 (2004)]. For our highest resolution and most accurate gauge, we estimate the duration of this data set's last orbit to be approximately 59MADM.

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Language(s): eng - English
 Dates: 2006
 Publication Status: Published in print
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 Identifiers: eDoc: 249144
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Title: The Fifteenth Workshop on General Relativity and Gravitation in Japan
Place of Event: Tokyo Institute of Technology, Tokyo, Japan
Start-/End Date: 2005-11-28 - 2005-12-02

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Title: Physical Review Letters
Source Genre: Journal
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Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 171 - 174 Identifier: -