旋转孤立视界的力学
广义相对论与量子宇宙学
2009-11-07 v2
摘要
黑洞力学 recently extended by replacing the more commonly used event horizons in stationary space-times with isolated horizons in more general space-times (which may admit radiation arbitrarily close to black holes). However, so far the detailed analysis has been restricted to non-rotating black holes (although it incorporated arbitrary distortion, as well as electromagnetic, Yang-Mills and dilatonic charges). We now fill this gap by first introducing the notion of isolated horizon angular momentum and then extending the first law to the rotating case.
引用
@article{arxiv.gr-qc/0103026,
title = {Mechanics of Rotating Isolated Horizons},
author = {Abhay Ashtekar and Christopher Beetle and Jerzy Lewandowski},
journal= {arXiv preprint arXiv:gr-qc/0103026},
year = {2009}
}
备注
31 pages REVTeX, 1 eps figure; Minor typos corrected and a footnote added