Cavaglià, Marco; Das, Saurya How classical are TeV-scale black holes. (English) Zbl 1060.83521 Classical Quantum Gravity 21, No. 19, 4511-4522 (2004). Summary: 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. Cited in 30 Documents MSC: 83C57 Black holes PDF BibTeX XML Cite \textit{M. Cavaglià} and \textit{S. Das}, Classical Quantum Gravity 21, No. 19, 4511--4522 (2004; Zbl 1060.83521) Full Text: DOI arXiv