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.
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Acknowledgments
The work of E.W. is supported by the Lancaster-Manchester-Sheffield Consortium for Fundamental Physics under STFC Grant ST/J000418/1. The work of P.K. has been co-financed by the European Union (European Social Fund—ESF) and Greek national funds through the Operational Program “Education and Lifelong Learning” of the National Strategic Reference Framework (NSRF)—Research Funding Program: “ARISTEIA. Investing in the society of knowledge through the European Social Fund”. Part of this work was supported by the COST Actions MP0905 “Black Holes in a Violent Universe” and MP1210 “The String Theory Universe”.
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Kanti, P., Winstanley, E. (2015). Hawking Radiation from Higher-Dimensional Black Holes. In: Calmet, X. (eds) Quantum Aspects of Black Holes. Fundamental Theories of Physics, vol 178. Springer, Cham. https://doi.org/10.1007/978-3-319-10852-0_8
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