Black Hole Decay Rates in Large Extra Dimensions

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dc.creatorCasadio, R.
dc.creatorHarms, B.
dc.date2001-06-06
dc.date.accessioned2026-07-25T17:01:47Z
dc.descriptionWe study the evaporation of black holes in space-times with extra dimensions of size L. We show that the luminosity is greatly damped when the horizon becomes smaller than L and black holes born with an initial size smaller than L are almost stable. This effect is due to the dependence of both the occupation number density of Hawking quanta and the grey-body factor of a black hole on the dimensionality of space.
dc.descriptionLaTeX2e with Rinton style, 4 pages, 2 figure EPS files, to appear in the Proceedings of PASCOS 2001
dc.identifierhttps://arxiv.org/abs/gr-qc/0106018
dc.identifierhttp://arxiv.org/abs/gr-qc/0106018
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/45123
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleBlack Hole Decay Rates in Large Extra Dimensions
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