Two physical characteristics of numerical apparent horizons

Details Two physical characteristics of numerical apparent horizons Two physical characteristics of numerical apparent horizons

2007-09-06

arxiv.org/abs/0709.0934v2

Can. J. Phys.86, 669-673 (2008)

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, 2 figures, conference proceedings loosely based on talk given at Theory Canada III (Edmonton, Alberta, 2007). V2: Min

Scientific paper

10.1139/P07-194

This article translates some recent results on quasilocal horizons into the
language of $(3+1)$ 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.

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