Numerical relativity in 3+1 dimensions

Brügmann, Bernd

doi:10.1002/(SICI)1521-3889(200005)9:3/5<227::AID-ANDP227>3.0.CO;2-D

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学術論文

Numerical relativity in 3+1 dimensions

MPS-Authors

Brügmann, Bernd
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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AnnalenderPhysik.9.3-5.pdf
(出版社版), 599KB

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引用

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.

引用: https://hdl.handle.net/11858/00-001M-0000-0013-6163-7

要旨

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.