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Phys. Rev. D 71, 124039 (2005) [6 pages]

Rotating black holes at future colliders. II. Anisotropic scalar field emission

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Daisuke Ida*
Department of Physics, Gakushuin University, Tokyo 171-8588, Japan

Kin-ya Oda†
Physikalisches Institut der Universität Bonn, Nussallee 12, Bonn 53115, Germany

Seong Chan Park‡
Institute for High Energy Phenomenology, Floyd R. Newman Laboratory for Elementary Particle Physics, Cornell University, Ithaca, New York 14853, USA

Received 7 March 2005; published 29 June 2005

This is the sequel to the first paper of the series, where we have discussed the Hawking radiation from five-dimensional rotating black holes for spin 0, 1/2, and 1 brane fields in the low frequency regime. We consider the emission of a brane-localized scalar field from rotating black holes in general space-time dimensions without relying on the low frequency expansions.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.71.124039
DOI:
10.1103/PhysRevD.71.124039
PACS:
04.50.+h, 04.70.Dy, 11.25.Mj, 11.25.Wx

*Electronic address: daisuke.ida@gakushuin.ac.jp

†Electronic address: odakin@th.physik.uni-bonn.de

‡Electronic address: spark@mail.lns.cornell.edu

 
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