三维黑洞的近视界动力学
高能物理 - 理论
2020-01-29 v4 广义相对论与量子宇宙学
摘要
我们在近视界边界条件所施加的约束下，对具有负宇宙学常数的三维爱因斯坦引力进行哈密顿约化。该理论约化为视界上的 Floreanini-Jackiw 型标量场论，其中标量零模捕获了全局黑洞电荷。近视界哈密顿量为全导数项，这解释了标量场所有振子模的柔软性。我们还发现了一族(Korteweg-de Vries)修正边界条件的层级，并用以解除视界上软毛激发的简并。
引用
@article{arxiv.1906.10694,
title = {Near horizon dynamics of three dimensional black holes},
author = {Daniel Grumiller and Wout Merbis},
journal= {arXiv preprint arXiv:1906.10694},
year = {2020}
}
备注
30pp, v2: added refs. and remark in discussion section, v3: extended and corrected first two paragraphs in section 2.2 and added last paragraph on near horizon nomenclature in section 2.3, v4: extended analysis to include dynamical holonomy