How classical are TeV-scale black holes?

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

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Bibliographic Details
Main Authors Cavaglia, Marco, Das, Saurya
Format Journal Article
LanguageEnglish
Published 06.04.2004
Subjects
Physics - General Relativity and Quantum Cosmology
Physics - High Energy Physics - Phenomenology
Physics - High Energy Physics - Theory
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Summary:Class.Quant.Grav. 21 (2004) 4511-4522 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.
DOI:10.48550/arxiv.hep-th/0404050