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.
Original language | English (US) |
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Article number | 072 |
Journal | Journal of High Energy Physics |
Volume | 2008 |
Issue number | 11 |
DOIs | |
State | Published - Nov 1 2008 |
Keywords
- Black holes
- Large extra dimensions
- Models of quantum gravity
ASJC Scopus subject areas
- Nuclear and High Energy Physics