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

Journal Article · Sat Aug 15 00:00:00 EDT 2009 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.80.045021· OSTI ID:21322517

Doukas, Jason ^[1]; Cho, H T ^[2]; Cornell, A S ^[3]; Naylor, Wade ^[4]

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1. Department of Mathematics and Statistics, University of Melbourne, Parkville, Victoria 3010 (Australia)
2. Department of Physics, Tamkang University, Tamsui, Taipei, Taiwan (China)
3. National Institute for Theoretical Physics, School of Physics, University of the Witwatersrand, Wits 2050 (South Africa)
4. 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

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BLACK HOLES
DE SITTER SPACE
EMISSION
GRAVITONS
KERR FIELD
MANY-DIMENSIONAL CALCULATIONS