Two physical characteristics of numerical apparent horizons
General Relativity and Quantum Cosmology
2009-11-13 v2
Abstract
This article translates some recent results on quasilocal horizons into the language of general relativity so as to make them more useful to numerical relativists. In particular quantities are described which characterize how quickly an apparent horizon is evolving and how close it is to either equilibrium or extremality.
Cite
@article{arxiv.0709.0934,
title = {Two physical characteristics of numerical apparent horizons},
author = {Ivan Booth},
journal= {arXiv preprint arXiv:0709.0934},
year = {2009}
}
Comments
6 pages, 2 figures, conference proceedings loosely based on talk given at Theory Canada III (Edmonton, Alberta, 2007). V2: Minor changes in response to referees comments to improve clarity and fix typos. One reference added