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  Gravitational collapse of gravitational waves in 3D numerical relativity.

Alcubierre, M., Allen, G., Brügmann, B., Lanfermann, G., Seidel, E., Suen, W.-M., et al. (2000). Gravitational collapse of gravitational waves in 3D numerical relativity. Physical Review D, 61(4): 041501. doi:10.1103/PhysRevD.61.041501.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-574E-6 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-574F-4
Genre: Journal Article

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Phy.Rev.D.61.041501.pdf (Publisher version), 69KB
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Alcubierre, Miguel1, Author
Allen, Gabrielle1, Author
Brügmann, Bernd1, Author
Lanfermann, Gerd1, Author
Seidel, Edward1, Author
Suen, Wai-Mo, Author
Tobias, Malcolm, Author
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1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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 Abstract: We demonstrate that evolutions of three-dimensional, strongly non-linear gravitational waves can be followed in numerical relativity, hence allowing many interesting studies of both fundamental and observational consequences. We study the evolution of time-symmetric, axisymmetric and non-axisymmetric Brill waves, including waves so strong that they collapse to form black holes under their own self-gravity. An estimate for the critical amplitude for black hole formation in a particular interpolating family of initial data is obtained. The gravitational waves emitted in the black hole formation process are compared to those emitted in the head-on collision of two Misner black holes.

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 Dates: 2000-02-15
 Publication Status: Issued
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 Identifiers: eDoc: 206100
URI: http://xxx.lanl.gov/archive/gr-qc/
Other: 27877
DOI: 10.1103/PhysRevD.61.041501
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Title: Physical Review D
Source Genre: Journal
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Pages: - Volume / Issue: 61 (4) Sequence Number: 041501 Start / End Page: - Identifier: ISSN: 0556-2821