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Discovery Reach for Black Hole Production

Models with extra space dimensions, in which our Universe exists on a 4-dimensional brane embedded in a higher dimensional bulk space-time, offer a new way to address outstanding problems in and beyond the Standard Model. In such models the Planck scale in the bulk can be of the order of the electro...

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Autor principal: The ATLAS collaboration
Lenguaje:eng
Publicado: 2009
Materias:
Acceso en línea:http://cds.cern.ch/record/1166305
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author The ATLAS collaboration
author_facet The ATLAS collaboration
author_sort The ATLAS collaboration
collection CERN
description Models with extra space dimensions, in which our Universe exists on a 4-dimensional brane embedded in a higher dimensional bulk space-time, offer a new way to address outstanding problems in and beyond the Standard Model. In such models the Planck scale in the bulk can be of the order of the electroweak symmetry breaking scale. This allows the coupling strength of gravity to increase to a size similar to the other interactions, opening the way to the unification of gravity and the gauge interactions. The increased strength of gravity in the bulk space-time means that quantum gravity effects would be observable in the TeV energy range reachable by the LHC. The most spectacular phenomenon would be the production of black holes, which would decay semi-classically by Hawking radiation emitting high energy particles. In this note, we discuss the potential for the ATLAS experiment to discover such black holes in the early data (1--1000 pb$^{-1}$).
id cern-1166305
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2009
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spelling cern-11663052021-04-18T19:40:03Zhttp://cds.cern.ch/record/1166305engThe ATLAS collaborationDiscovery Reach for Black Hole ProductionDetectors and Experimental TechniquesModels with extra space dimensions, in which our Universe exists on a 4-dimensional brane embedded in a higher dimensional bulk space-time, offer a new way to address outstanding problems in and beyond the Standard Model. In such models the Planck scale in the bulk can be of the order of the electroweak symmetry breaking scale. This allows the coupling strength of gravity to increase to a size similar to the other interactions, opening the way to the unification of gravity and the gauge interactions. The increased strength of gravity in the bulk space-time means that quantum gravity effects would be observable in the TeV energy range reachable by the LHC. The most spectacular phenomenon would be the production of black holes, which would decay semi-classically by Hawking radiation emitting high energy particles. In this note, we discuss the potential for the ATLAS experiment to discover such black holes in the early data (1--1000 pb$^{-1}$).ATL-PHYS-PUB-2009-074ATL-COM-PHYS-2009-097oai:cds.cern.ch:11663052009-03-11
spellingShingle Detectors and Experimental Techniques
The ATLAS collaboration
Discovery Reach for Black Hole Production
title Discovery Reach for Black Hole Production
title_full Discovery Reach for Black Hole Production
title_fullStr Discovery Reach for Black Hole Production
title_full_unstemmed Discovery Reach for Black Hole Production
title_short Discovery Reach for Black Hole Production
title_sort discovery reach for black hole production
topic Detectors and Experimental Techniques
url http://cds.cern.ch/record/1166305
work_keys_str_mv AT theatlascollaboration discoveryreachforblackholeproduction