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How classical are TeV-scale black holes?

Marco Cavaglià et al 2004 Class. Quantum Grav. 21 4511-4522   doi: 10.1088/0264-9381/21/19/001  Help

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Marco Cavaglià1 and Saurya Das2
1 Department of Physics and Astronomy, The University of Mississippi, PO Box 1848, University, MS 38677-1848, USA
2 Department of Physics, University of Lethbridge, 4401 University Drive, Lethbridge, Alberta T1K 3M4, Canada
E-mail: cavaglia@phy.olemiss.edu and saurya.das@uleth.ca

Abstract. 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 numbers: 04.70.Dy, 04.80.Cc, 03.65.Ta

Print publication: Issue 19 (7 October 2004)
Received 13 April 2004, in final form 2 August 2004
Published 14 September 2004

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