Numerical Relativity in 3+1 Dimensions
General Relativity and Quantum Cosmology
2017-09-27 v1
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.
Cite
@article{arxiv.gr-qc/9912009,
title = {Numerical Relativity in 3+1 Dimensions},
author = {Bernd Bruegmann},
journal= {arXiv preprint arXiv:gr-qc/9912009},
year = {2017}
}
Comments
23 pages, 5 figures, review talk for Journees Relativistes 1999