Kanti, P. and Winstanley, E. orcid.org/0000-0001-8964-8142 (2014) Hawking Radiation from Higher-Dimensional Black Holes. Fundamental Theories of Physics, 178. pp. 229-265. ISSN 0168-1222
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.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2015 Springer International Publishing Switzerland. This is an author produced version of a paper subsequently published in Fundamental Theories of Physics. Uploaded in accordance with the publisher's self-archiving policy. |
Keywords: | hep-th; hep-th; astro-ph.CO; gr-qc; hep-ph |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield) |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 19 May 2016 11:11 |
Last Modified: | 21 Mar 2018 20:04 |
Published Version: | http://dx.doi.org/10.1007/978-3-319-10852-0_8 |
Status: | Published |
Publisher: | Springer Verlag |
Refereed: | Yes |
Identification Number: | 10.1007/978-3-319-10852-0_8 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:98090 |