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arXiv · 0906.1515

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

Jason Doukas·H. T. Cho·A. S. Cornell·Wade Naylor
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Abstract

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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Jason Doukas, H. T. Cho, A. S. Cornell, Wade Naylor. 2009-07-01. Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes. https://doi.org/10.1103/physrevd.80.045021

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