Phenomenology of black hole evaporation with a cosmological constant

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dc.creatorLabbe, J.
dc.creatorBarrau, A.
dc.creatorGrain, J.
dc.date2005-11-17
dc.date.accessioned2026-07-07T11:43:36Z
dc.date.available2026-07-07T11:43:36Z
dc.descriptionIn this brief note, we investigate some possible experimental consequences of the de-Sitter or Anti-de-Sitter background spacetime structure for d-dimensional evaporating black holes. Possible observational signatures in Large Hadron Collider (LHC) events are considered in the framework of the Arkani-Hamed-Dimopoulos-Dvali (ADD) braneworld model. Lower bounds on the value of the bulk cosmological constant required to produce visible effects are derived thanks to a dynamical Monte-Carlo simulation. This preliminary study has to be refined by the accurate computation of the greybody factors. It opens a new way to investigate the structure of non-asymptotically flat higher-dimensional spacetimes.
dc.descriptionProceedings of the HEP2005 conference. Related greybody factors for evaporating black holes available at : http://lpsc.in2p3.fr/ams/greybody/
dc.identifierhttps://arxiv.org/abs/hep-ph/0511211
dc.identifierhttp://arxiv.org/abs/hep-ph/0511211
dc.identifierPoSHEP2005:013,2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201295
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Experiment
dc.subjectHigh Energy Physics - Theory
dc.titlePhenomenology of black hole evaporation with a cosmological constant
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