Calculable Corrections to Brane Black Hole Decay; 1, The Scalar Case

In the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections...

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Detalles Bibliográficos
Autores principales: Kanti, Panagiota, March-Russell, John
Lenguaje:eng
Publicado: 2002
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.66.024023
http://cds.cern.ch/record/544586
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author Kanti, Panagiota
March-Russell, John
author_facet Kanti, Panagiota
March-Russell, John
author_sort Kanti, Panagiota
collection CERN
description In the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections to the energy spectrum (the greybody factors) for decay into scalar fields, as a function of the number of toroidally compactified extra dimensions, and partial wave number.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2002
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spelling cern-5445862023-10-04T06:31:59Zdoi:10.1103/PhysRevD.66.024023http://cds.cern.ch/record/544586engKanti, PanagiotaMarch-Russell, JohnCalculable Corrections to Brane Black Hole Decay; 1, The Scalar CaseParticle Physics - PhenomenologyIn the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections to the energy spectrum (the greybody factors) for decay into scalar fields, as a function of the number of toroidally compactified extra dimensions, and partial wave number.In the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections to the energy spectrum (the greybody factors) for decay into scalar fields, as a function of the number of toroidally compactified extra dimensions, and partial wave number.hep-ph/0203223CERN-TH-2002-014CERN-TH-2002-014oai:cds.cern.ch:5445862002-03-22
spellingShingle Particle Physics - Phenomenology
Kanti, Panagiota
March-Russell, John
Calculable Corrections to Brane Black Hole Decay; 1, The Scalar Case
title Calculable Corrections to Brane Black Hole Decay; 1, The Scalar Case
title_full Calculable Corrections to Brane Black Hole Decay; 1, The Scalar Case
title_fullStr Calculable Corrections to Brane Black Hole Decay; 1, The Scalar Case
title_full_unstemmed Calculable Corrections to Brane Black Hole Decay; 1, The Scalar Case
title_short Calculable Corrections to Brane Black Hole Decay; 1, The Scalar Case
title_sort calculable corrections to brane black hole decay; 1, the scalar case
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.66.024023
http://cds.cern.ch/record/544586
work_keys_str_mv AT kantipanagiota calculablecorrectionstobraneblackholedecay1thescalarcase
AT marchrusselljohn calculablecorrectionstobraneblackholedecay1thescalarcase

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