Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes
Abstract
In this article we present results for tensor graviton modes (in seven dimensions and greater, n≥ 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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