Numerical Relativity in 3+1 Dimensions
arXiv:gr-qc/9912009 · doi:10.1002/(SICI)1521-3889(200005)9:3/5<227::AID-ANDP227>3.0.CO;2-D
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.
23 pages, 5 figures, review talk for Journees Relativistes 1999
References in corpus (3)
Cited by in corpus (11)
- Gauge conditions for long-term numerical black hole evolutions without excision
- Numerical Relativity: A review
- Simple excision of a black hole in 3+1 numerical relativity
- The 3D Grazing Collision of Two Black Holes
- Binary black hole initial data for numerical general relativity based on post-Newtonian data
- Dynamical evolution of quasi-circular binary black hole data
- Evolving spherical boson stars on a 3D cartesian grid
- The Search for Gravitational Waves
- Gauge conditions for binary black hole puncture data based on an approximate helical Killing vector
- Maximal Slicing for Puncture Evolutions of Schwarzschild and Reissner-Nordström Black Holes
- Energy and angular momentum radiated for non head-on binary black hole collisions