How classical are TeV-scale black holes?

Cavagalià, Marco; Das, Saurya

How classical are TeV-scale black holes?

dc.contributor.author	Cavagalià, Marco
dc.contributor.author	Das, Saurya
dc.date.accessioned	2015-12-23T17:05:51Z
dc.date.available	2015-12-23T17:05:51Z
dc.date.issued	2015-12-23
dc.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.”	en_US
dc.description.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.	en_US
dc.description.peer-review	No	en_US
dc.identifier.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
dc.identifier.uri	https://hdl.handle.net/10133/3852
dc.language.iso	en_CA	en_US
dc.publisher.department	Department of Physics	en_US
dc.publisher.faculty	Arts and Science	en_US
dc.publisher.institution	University of Mississippi	en_US
dc.publisher.institution	University of Lethbridge	en_US
dc.publisher.url	https://doi.org/10.1088/0264-9381/21/19/001
dc.subject	Hawking temperature	en_US
dc.subject	Entropy	en_US
dc.subject	Black holes	en_US
dc.subject	Generalized uncertainty principle	en_US
dc.subject	Thermal fluctuations	en_US
dc.subject	TeV scale	en_US
dc.title	How classical are TeV-scale black holes?	en_US
dc.type	Article	en_US