Hawking Radiation from Higher-Dimensional Black Holes
arXiv:1402.3952 · doi:10.1007/978-3-319-10852-0_8
Abstract
We review the quantum field theory description of Hawking radiation from evaporating black holes and summarize what is known about Hawking radiation from black holes in more than four space-time dimensions. In the context of the Large Extra Dimensions scenario, we present the theoretical formalism for all types of emitted fields and a selection of results on the radiation spectra. A detailed analysis of the Hawking fluxes in this case is essential for modelling the evaporation of higher-dimensional black holes at the LHC, whose creation is predicted by low-energy models of quantum gravity. We discuss the status of the quest for black-hole solutions in the context of the Randall-Sundrum brane-world model and, in the absence of an exact metric, we review what is known about Hawking radiation from such black holes.
Latex2e file, 35 pages, 14 figures, references added, typos corrected, To be published in "Quantum Aspects of Black Holes", ed. X. Calmet (Springer, 2014)
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