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  Binary black hole initial data for numerical general relativity based on post-Newtonian data

Tichy, W., Brügmann, B., Campanelli, M., & Diener, P. (2003). Binary black hole initial data for numerical general relativity based on post-Newtonian data. Physical Review D, 67(6): 064008.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-527F-6 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-5280-D
Genre: Journal Article

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Tichy, Wolfgang1, Author
Brügmann, Bernd1, Author
Campanelli, Manuela1, Author
Diener, Peter1, Author
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1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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 Abstract: With the goal of taking a step toward the construction of astrophysically realistic initial data for numerical simulations of black holes, we for the first time derive a family of fully general relativistic initial data based on post-2-Newtonian expansions of the 3-metric and extrinsic curvature without spin. It is expected that such initial data provide a direct connection with the early inspiral phase of the binary system. We discuss a straightforward numerical implementation, which is based on a generalized puncture method. Furthermore, we suggest a method to address some of the inherent ambiguity in mapping post-Newtonian data onto a solution of the general relativistic constraints

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 Dates: 2003
 Publication Status: Issued
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 Identifiers: eDoc: 3086
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Title: Physical Review D
Source Genre: Journal
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Pages: - Volume / Issue: 67 (6) Sequence Number: 064008 Start / End Page: - Identifier: -