Skip to main content
Article thumbnail
Location of Repository

Angular profile of emission of non-zero spin fields from a higher-dimensional black hole

By M. Casals, S.R. Dolan, P. Kanti and E. Winstanley

Abstract

Recent works have included the effect of rotation on simulations of black hole events at the LHC, showing that the angular momentum of the black hole cannot be ignored and it makes a non-trivial contribution for most of the lifetime of the black hole. A key consequence of the rotation of the black hole is that the Hawking radiation is no longer isotropic, making it more difficult to infer space–time parameters from measurements of the emitted particles. In this Letter we study the angular distribution of the Hawking emission of non-zero spin particles with specific helicity on the brane. We argue that the shape of the distribution could be used as a measure of the angular momentum of the black hole.\ud \u

Publisher: Elsevier
Year: 2009
OAI identifier: oai:eprints.whiterose.ac.uk:10550

Suggested articles


To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request.