The decay-time of non-commutative micro-black holes

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dc.creatorCasadio, Roberto
dc.creatorNicolini, Piero
dc.date2008-09-15
dc.date.accessioned2026-07-07T12:56:42Z
dc.date.available2026-07-07T12:56:42Z
dc.descriptionNon-commutative black holes are characterised by a minimum mass which would result in a remnant after the Hawking evaporation ends. We numerically study the decay of neutral non-commutative black holes for up to ten spatial dimensions and typical parameters that would make their production possible at the LHC. Neglecting possible accretion mechanism, we find that decay-times are extremely short.
dc.descriptionLatex, 8 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0809.2471
dc.identifierhttp://arxiv.org/abs/0809.2471
dc.identifierJHEP 0811:072,2008
dc.identifierdoi:10.1088/1126-6708/2008/11/072
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224672
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe decay-time of non-commutative micro-black holes
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