How classical are TeV-scale black holes?

Details How classical are TeV-scale black holes? How classical are TeV-scale black holes?

2004-04-06

arxiv.org/abs/hep-th/0404050v2

Class.Quant.Grav. 21 (2004) 4511-4522

Physics

High Energy Physics

High Energy Physics - Theory

10 pages, no figures, REVTeX style. Extra comments and references to match version accepted to Classical and Quantum Gravity

Scientific paper

10.1088/0264-9381/21/19/001

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.

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