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  The Current Status of Binary Black Hole Simulations in Numerical Relativity

Hinder, I. (2010). The Current Status of Binary Black Hole Simulations in Numerical Relativity. Classical and quantum gravity, 27(11): 114004. doi:10.1088/0264-9381/27/11/114004.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0012-652A-B Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0012-652C-7
Genre: Journal Article

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1001.5161 (Preprint), 300KB
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 Creators:
Hinder, Ian1, Author           
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1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: Since the breakthroughs in 2005 which have led to long term stable solutions of the binary black hole problem in numerical relativity, much progress has been made. I present here a short summary of the state of the field, including the capabilities of numerical relativity codes, recent physical results obtained from simulations, and improvements to the methods used to evolve and analyse binary black hole spacetimes.

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 Dates: 2010-01-282010
 Publication Status: Issued
 Pages: 14 pages; submitted to the Classical and Quantum Gravity special issue for NRDA2009
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 Rev. Type: -
 Identifiers: arXiv: 1001.5161
DOI: 10.1088/0264-9381/27/11/114004
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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics
Pages: - Volume / Issue: 27 (11) Sequence Number: 114004 Start / End Page: - Identifier: Other: 954925513480
Other: 0264-9381