Numerical evidences for the angular momentum-mass inequality for multiple axially symmetric black holes
General Relativity and Quantum Cosmology
2010-05-12 v1
Abstract
We present numerical evidences for the validity of the inequality between the total mass and the total angular momentum for multiple axially symmetric (non-stationary) black holes. We use a parabolic heat flow to solve numerically the stationary axially symmetric Einstein equations. As a by product our method, we also give numerical evidences that there are no regular solutions of Einstein equations that describe two extreme, axially symmetric black holes in equilibrium.
Keywords
Cite
@article{arxiv.0905.0708,
title = {Numerical evidences for the angular momentum-mass inequality for multiple axially symmetric black holes},
author = {Sergio Dain and Omar Ortiz},
journal= {arXiv preprint arXiv:0905.0708},
year = {2010}
}
Comments
16 pages, 10 figures