Hawking Radiation from Higher-Dimensional Black Holes
  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.
