How classical are TeV-scale black holes?
高能物理 - 理论
2009-11-10 v2 广义相对论与量子宇宙学
高能物理 - 唯象学
摘要
We show that the Hawking temperature and the entropy of black holes are subject to corrections from two sources: the generalized uncertainty principle and thermal fluctuations. Both effects increase the temperature and decrease the entropy, resulting in faster decay and ``less classical'' black holes. We discuss the implications of these results for TeV-scale black holes that are expected to be produced at future colliders.
引用
@article{arxiv.hep-th/0404050,
title = {How classical are TeV-scale black holes?},
author = {Marco Cavaglia and Saurya Das},
journal= {arXiv preprint arXiv:hep-th/0404050},
year = {2009}
}
备注
10 pages, no figures, REVTeX style. Extra comments and references to match version accepted to Classical and Quantum Gravity