包含畸变与旋转的量子几何与黑洞熵
广义相对论与量子宇宙学
2009-11-11 v3
摘要
黑洞的平衡状态可由孤立边界模型。若其内在几何为球形，称为 I 类；若其为轴对称，称为 II 类。量子类型 I 边界几何的详细理论及其熵的计算可推广至类型 II，从而包含任意畸变和旋转。大尺度边界的熵主导项仍由其引力面积的四分之一给出，其 Barbero-Immirzi 参数与 I 类情况相同。概述其扩展思想与构建方法。
关键词
引用
@article{arxiv.gr-qc/0509033,
title = {Quantum geometry and black hole entropy: inclusion of distortion and rotation},
author = {Jonathan Engle},
journal= {arXiv preprint arXiv:gr-qc/0509033},
year = {2009}
}
备注
Text based on parallel talk given at the VI Mexican School on Gravitation and Mathematical Physics: ``Approaches to Quantum Gravity'', held in Playa del Carmen, Mexico, in November of 2004; IGPG preprint number added; metadata abstract corrected