Probing quantum gravity effects in black holes at LHC
arXiv:hep-ph/0601243
Abstract
We study modifications of the Hawking emission in the evaporation of miniature black holes possibly produced in accelerators when their mass approaches the fundamental scale of gravity, set to 1 TeV according to some extra dimension models. Back-reaction and quantum gravity corrections are modelled by employing modified relations between the black hole mass and temperature. We release the assumption that black holes explode at 1 TeV or leave a remnant, and let them evaporate to much smaller masses. We have implemented such modified decay processes into an existing micro-black hole event generator, performing a study of the decay products in order to search for phenomenological evidence of quantum gravity effects.
7 pages, 4 figures
Cited by in corpus (9)
- Non-commutative geometry inspired higher-dimensional charged, black holes
- Catfish: A Monte Carlo simulator for black holes at the LHC
- Quantum Gravity Effects in Black Holes at the LHC
- Black hole evaporation in a spherically symmetric non-commutative space-time
- Gravitational amplitudes in black-hole evaporation: the effect of non-commutative geometry
- Comparison of Black Hole Generators for the LHC
- Mini Black Holes at the LHC: Discovery Through Di-Jet Suppression, Mono-Jet Emission and a Supersonic Boom in the Quark-Gluon Plasma in ALICE, ATLAS and CMS
- The Method of Comparison Equations for Schwarzschild Black Holes
- Particle Phenomenology of Gravitational Events at the TeV Scale