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Black Holes at the LHC

If the scale of quantum gravity is near a TeV, the LHC will be producing one black hole (BH) about every second. The BH decays into prompt, hard photons and charged leptons is a clean signature with low background. The absence of significant missing energy allows the reconstruction of the mass of th...

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Detalles Bibliográficos
Autores principales: Dimopoulos, Savas K, Landsberg, G L
Lenguaje:eng
Publicado: 2001
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevLett.87.161602
http://cds.cern.ch/record/506130
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author Dimopoulos, Savas K
Landsberg, G L
author_facet Dimopoulos, Savas K
Landsberg, G L
author_sort Dimopoulos, Savas K
collection CERN
description If the scale of quantum gravity is near a TeV, the LHC will be producing one black hole (BH) about every second. The BH decays into prompt, hard photons and charged leptons is a clean signature with low background. The absence of significant missing energy allows the reconstruction of the mass of the decaying BH. The correlation between the BH mass and its temperature, deduced from the energy spectrum of the decay products, can test experimentally the higher dimensional Hawking evaporation law. It can also determine the number of large new dimensions and the scale of quantum gravity.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2001
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spelling cern-5061302019-09-30T06:29:59Zdoi:10.1103/PhysRevLett.87.161602http://cds.cern.ch/record/506130engDimopoulos, Savas KLandsberg, G LBlack Holes at the LHCParticle Physics - PhenomenologyIf the scale of quantum gravity is near a TeV, the LHC will be producing one black hole (BH) about every second. The BH decays into prompt, hard photons and charged leptons is a clean signature with low background. The absence of significant missing energy allows the reconstruction of the mass of the decaying BH. The correlation between the BH mass and its temperature, deduced from the energy spectrum of the decay products, can test experimentally the higher dimensional Hawking evaporation law. It can also determine the number of large new dimensions and the scale of quantum gravity.hep-ph/0106295ITP-2001-31oai:cds.cern.ch:5061302001-06-27
spellingShingle Particle Physics - Phenomenology
Dimopoulos, Savas K
Landsberg, G L
Black Holes at the LHC
title Black Holes at the LHC
title_full Black Holes at the LHC
title_fullStr Black Holes at the LHC
title_full_unstemmed Black Holes at the LHC
title_short Black Holes at the LHC
title_sort black holes at the lhc
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevLett.87.161602
http://cds.cern.ch/record/506130
work_keys_str_mv AT dimopoulossavask blackholesatthelhc
AT landsberggl blackholesatthelhc