Footprints of Higher-Dimensional Decaying Black Holes

Abstract

We review the current results for the emission of Hawking radiation by a higher-dimensional black hole during the Schwarzschild and the spin-down phases. We discuss particularly the role of the angular variation of the emitted radiation on the brane during the latter phase, the radiation spectra for gravitons in the bulk, and the effect of the mass of the emitted particles in determining the bulk-to-brane energy balance.

arXiv commentLatex file, 15 Pages, 7 Figures, invited talk at the SEENET-MTP Workshop 2011 "Particle Physics from TeV to Planck Scale", 28 August-1 September 2011, Donji Milanovac, Serbia, to appear in the proceedings

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