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dc.contributor.authorEmparan García de Salazar, Roberto
dc.contributor.authorHorowitz, Gary
dc.contributor.authorMyers, Robert Charlescat
dc.description.abstractWe examine the evaporation of a small black hole on a brane in a world with large extra dimensions. Since the masses of many Kaluza-Klein modes are much smaller than the Hawking temperature of the black hole, it has been claimed that most of the energy is radiated into these modes. We show that this is incorrect. Most of the energy goes into the modes on the brane. This raises the possibility of observing Hawking radiation in future high energy colliders if there are large extra dimensions.eng
dc.format.extent4 p.-
dc.publisherAmerican Physical Societycat
dc.relation.isformatofReproducció digital del document proporcionada per PROLA i
dc.relation.ispartofPhysical Review Letters, 2000, vol. 85, núm. 3, p. 499-502cat
dc.rights(c) American Physical Society, 2000cat
dc.sourceArticles publicats en revistes (Física de la Matèria Condensada)-
dc.subject.classificationRelativitat (Física)cat
dc.subject.classificationTeoria de camps (Física)cat
dc.subject.classificationForats negres (Astronomia)cat
dc.subject.otherGeneral relativity and gravitationeng
dc.subject.otherGeneral theory of fields and particleseng
dc.subject.otherBlack holes (Astronomy)eng
dc.titleBlack holes radiate mainly on the braneeng
Appears in Collections:Articles publicats en revistes (Física de la Matèria Condensada)

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