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BLACK HOLES IN THEORIES WITH LARGE EXTRA DIMENSIONS: A REVIEW

KANTI, PANAGIOTA·2004·International Journal of Modern Physics A
DOI 10.1142/s0217751x04018324
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Abstract

We start by reviewing the existing literature on the creation of black holes during high-energy particle collisions, both in the absence and in the presence of extra, compact, spacelike dimensions. Then, we discuss in detail the properties of the produced higher-dimensional black holes, namely the horizon radius, temperature and life-time, as well as the physics that governs the evaporation of these objects, through the emission of Hawking radiation. We first study the emission of visible Hawking radiation on the brane: we derive a master equation for the propagation of fields with arbitrary spin in the induced-on-the-brane black hole background, and we review all existing results in the literature for the emission of scalars, fermions and gauge bosons during the spin-down and Schwarzschild phases of the life of the black hole. Both analytical and numerical results for the graybody factors and radiation spectra are reviewed and exact results for the number and type of fields emitted on the brane as a function of the dimensionality of space–time are discussed. We finally study the emission of Hawking radiation in the bulk: graybody factors and radiation spectra are presented for the emission of scalar modes, and the ratio of the missing energy over the visible one is calculated for different values of the number of extra dimensions.

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  • The Hawking temperature of the higher dimensional black hole is T_H = (D-3)/(4πr+).

    “Meanwhile the Hawking temperature of the higher dimensional black hole is [63,64] T H = (D -3) 4πr + (C.8)”

    From Vacuum metastability with black holes (2015) · cites this paper as [64]

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Metadata

Authors
KANTI, P.
Venue
International Journal of Modern Physics A
Publisher
World Scientific Pub Co Pte Ltd
Published
2004-11-20
Volume
19
Issue
29
Pages
4899-4951
ISSN
  • 0217-751X
  • 1793-656X
DOI
10.1142/s0217751x04018324
Cited by
403
References
4
Language
en

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