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  Details on the gravitational-wave emission from rotating gravitational collapse in 3D

Baiotti, L., Hawke, I., Rezzolla, L., & Schnetter, E. (2007). Details on the gravitational-wave emission from rotating gravitational collapse in 3D. Journal of Physics: Conference Series, 66(1): 012045. doi:10.1088/1742-6596/66/1/012045.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0012-C3A3-1 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0012-C3A4-0
Genre: Journal Article

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 Creators:
Baiotti, Luca, Author
Hawke, Ian, Author
Rezzolla, Luciano1, Author           
Schnetter, Erik, Author
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1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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 Abstract: We here provide details on the numerical study of the gravitational-wave emission from the gravitational collapse to black holes of rotating neutron stars in three dimensions. More specifically, we concentrate on the use of mesh-refined grids, either fixed or progressive, as well as on the use of the excision techniques and of the advantages that result when this is not employed.

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 Dates: 2007
 Publication Status: Issued
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 Identifiers: DOI: 10.1088/1742-6596/66/1/012045
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Title: Journal of Physics: Conference Series
Source Genre: Journal
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Pages: - Volume / Issue: 66 (1) Sequence Number: 012045 Start / End Page: - Identifier: Other: 111097776606042
Other: 1742-6588