How Classical Are TeV-Scale Black Holes?
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.
M. Cavaglia and S. Das, "How Classical Are TeV-Scale Black Holes?," Classical and Quantum Gravity, vol. 21, no. 19, pp. 4511 - 4522, Institute of Physics - IOP Publishing, Sep 2004.
The definitive version is available at https://doi.org/10.1088/0264-9381/21/19/001
Natural Sciences and Engineering Research Council of Canada
University of Lethbridge.
International Standard Serial Number (ISSN)
Article - Journal
© 2004 Institute of Physics - IOP Publishing, All rights reserved.
01 Sep 2004
This work was supported in part by the Natural Sciences and Engineering Research Council of Canada and funds of the University of Lethbridge.