Spacetimes containing slowly evolving horizons
广义相对论与量子宇宙学
2011-07-19 v3
摘要
Slowly evolving horizons are trapping horizons that are "almost" isolated horizons. This paper reviews their definition and discusses several spacetimes containing such structures. These include certain Vaidya and Tolman-Bondi solutions as well as (perturbatively) tidally distorted black holes. Taking into account the associated mass scales, they also suggest that slowly evolving horizons are the norm rather than the exception in astrophysical processes that involve stellar-scale black holes.
引用
@article{arxiv.gr-qc/0603074,
title = {Spacetimes containing slowly evolving horizons},
author = {W. Kavanagh and I. Booth},
journal= {arXiv preprint arXiv:gr-qc/0603074},
year = {2011}
}
备注
14 pages, 2 figures, small changes which are mainly clarifications to the perturbed Schwarzschild section, final version to appear in PRD