Remarks on numerical relativity, geodesic motions, binary neutron star evolution
General Physics
2012-11-28 v1
Abstract
The computations of numerical relativity make use of (3+1)- decompositions of Einstein field equations. We examine the conceptual characteristics of this method; instances of compact-star binaries are considered. The preeminent role of the geodesic motions is emphasized.
Keywords
Cite
@article{arxiv.1211.6152,
title = {Remarks on numerical relativity, geodesic motions, binary neutron star evolution},
author = {A. Loinger and T. Marsico},
journal= {arXiv preprint arXiv:1211.6152},
year = {2012}
}
Comments
8 pages