Calculable Corrections to Brane Black Hole Decay I: The Scalar Case

Details Calculable Corrections to Brane Black Hole Decay I: The Scalar Case Calculable Corrections to Brane Black Hole Decay I: The Scalar Case

2002-03-22

arxiv.org/abs/hep-ph/0203223v2

Phys.Rev. D66 (2002) 024023

Physics

High Energy Physics

High Energy Physics - Phenomenology

Latex, 16 pages, typos fixed, references added

Scientific paper

10.1103/PhysRevD.66.024023

In the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections to the energy spectrum (the greybody factors) for decay into scalar fields, as a function of the number of toroidally compactified extra dimensions, and partial wave number.

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