How classical are TeV-scale black holes?
Date
2015-12-23
Authors
Cavagalià, Marco
Das, Saurya
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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.
Description
Sherpa Romeo green journal. “This is an author-created, un-copyedited version of an article accepted for publication/published in Classical and Quantum Gravity. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it.”
Keywords
Hawking temperature , Entropy , Black holes , Generalized uncertainty principle , Thermal fluctuations , TeV scale
Citation
Cavaglia, M., & Das, S. (2004). How classical are TeV-scale black holes? Classical and Quantum Gravity, 21(19), 4511-4522. https://doi.org/10.1088/0264-9381/21/19/001