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

doi:10.1103/PhysRevD.80.045021

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

Research output: Contribution to journal › Article › peer-review

26 Citations (Scopus)

Abstract

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.

Original language	English
Article number	045021
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	80
Issue number	4
DOIs	https://doi.org/10.1103/PhysRevD.80.045021
Publication status	Published - 20 Aug 2009
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics
Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.80.045021

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abstract = "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.",

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AU - Cornell, A. S.

AU - Naylor, Wade

PY - 2009/8/20

Y1 - 2009/8/20

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AB - 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.

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DO - 10.1103/PhysRevD.80.045021

M3 - Article

AN - SCOPUS:70049084801

SN - 1550-7998

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JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

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

Abstract

ASJC Scopus subject areas

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