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How classical are TeV-scale black holes?

Marco Cavaglià1 and Saurya Das2

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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.


PACS

04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics

04.80.Cc Experimental tests of gravitational theories

04.60.-m Quantum gravity

MSC

82B30 Statistical thermodynamics (See also 80-XX)

83C57 Black holes

Subjects

Gravitation and cosmology

Dates

Issue 19 (7 October 2004)

Received 13 April 2004, in final form 2 August 2004

Published 14 September 2004



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