Black Holes Radiate Mainly on the Brane

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dc.creatorEmparan, Roberto
dc.creatorHorowitz, Gary T.
dc.creatorMyers, Robert C.
dc.date2000-03-14
dc.date2000-06-06
dc.date.accessioned2026-07-07T10:53:20Z
dc.date.available2026-07-07T10:53:20Z
dc.descriptionWe 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.
dc.description11 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0003118
dc.identifierhttp://arxiv.org/abs/hep-th/0003118
dc.identifierPhys.Rev.Lett.85:499-502,2000
dc.identifierdoi:10.1103/PhysRevLett.85.499
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185448
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleBlack Holes Radiate Mainly on the Brane
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