Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes
Journal Article
·
· Physical Review. D, Particles Fields
- Department of Mathematics and Statistics, University of Melbourne, Parkville, Victoria 3010 (Australia)
- Department of Physics, Tamkang University, Tamsui, Taipei, Taiwan (China)
- National Institute for Theoretical Physics, School of Physics, University of the Witwatersrand, Wits 2050 (South Africa)
- Department of Physics, Ritsumeikan University, Kusatsu, Shiga 525-8577 (Japan)
In this article we present results for tensor graviton modes (in seven dimensions and greater, n{>=}3) for gray-body factors of Kerr-de Sitter 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-de Sitter black hole, we present some preliminary results for emissions assuming the standard Hawking normalization and a Bousso-Hawking-like normalization.
- OSTI ID:
- 21322517
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 80, Issue 4; Other Information: DOI: 10.1103/PhysRevD.80.045021; (c) 2009 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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