Non-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.
R. Casadio, P. Nicolini (2008). The decay-time of non-commutative micro-black holes. JOURNAL OF HIGH ENERGY PHYSICS, 11, 072-072 [10.1088/1126-6708/2008/11/072].
The decay-time of non-commutative micro-black holes
CASADIO, ROBERTO;
2008
Abstract
Non-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.File in questo prodotto:
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