Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes

Details Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes

2009-06-08

arxiv.org/abs/0906.1515v2

Phys.Rev.D80:045021,2009

Physics

High Energy Physics

High Energy Physics - Theory

12 pages, 18 figures

Scientific paper

10.1103/PhysRevD.80.045021

In this article we present results for tensor graviton modes (in seven dimensions and greater, $n\geq 3$) for greybody factors of Kerr-dS black holes and for Hawking radiation from simply rotating (n+4)-dimensional Kerr black holes. Although there is some subtlety with defining the Hawking temperature of a Kerr-dS black hole, we present some preliminary results for emissions assuming the standard Hawking normalization and a Bousso-Hawking-like normalization.

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