Black hole interior from loop quantum gravity
广义相对论与量子宇宙学
2009-07-24 v2 高能物理 - 理论
摘要
In this paper we calculate modifications to the Schwarzschild solution by using a semiclassical analysis of loop quantum black hole. We obtain a metric inside the event horizon that coincides with the Schwarzschild solution near the horizon but that is substantially different at the Planck scale. In particular we obtain a bounce of the two-sphere for a minimum value of the radius and that it is possible to have another event horizon close to the r=0 point.
引用
@article{arxiv.gr-qc/0611043,
title = {Black hole interior from loop quantum gravity},
author = {Leonardo Modesto},
journal= {arXiv preprint arXiv:gr-qc/0611043},
year = {2009}
}
备注
12 pages, 7 figures. Advances in High Energy Physics Volume 2008 (2008), Article ID 459290