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  Numerical relativity in 3+1 dimensions

Brügmann, B. (2000). Numerical relativity in 3+1 dimensions. Annalen der Physik, 9(3-5), 227-246. doi:10.1002/(SICI)1521-3889(200005)9:3/5<227:AID-ANDP227>3.0.CO;2-D.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-6163-7 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-6164-5
Genre: Journal Article

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AnnalenderPhysik.9.3-5.pdf (Publisher version), 599KB
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 Creators:
Brügmann, Bernd1, Author
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1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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 Abstract: Numerical relativity is finally approaching a state where the evolution of rather general (3+1)-dimensional data sets can be computed in order to solve the Einstein equations. After a general introduction, three topics of current interest are briefly reviewed: binary black hole mergers, the evolution of strong gravitational waves, and shift conditions for neutron star binaries.

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Language(s): eng - English
 Dates: 2000
 Publication Status: Published in print
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Title: Annalen der Physik
Source Genre: Journal
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Pages: - Volume / Issue: 9 (3-5) Sequence Number: - Start / End Page: 227 - 246 Identifier: ISSN: 0003-3804