2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/33921We 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.LaTeX2e with Rinton style, 4 pages, 2 figure EPS files, to appear in the Proceedings of PASCOS 2001General Relativity and Quantum CosmologyAstrophysicsHigh Energy Physics - Theorytext