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

淡江大學機構典藏 > 理學院 > 物理學系暨研究所 > 期刊論文 > Item 987654321/58298

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题名:	Graviton emission from simply rotating Kerr-de Sitter black holes: Transverse traceless tensor graviton modes
作者:	Doukas, Jason;Cho, H. T.;Cornell, A. S.;Naylor, Wade
贡献者:	淡江大學物理學系
日期:	2009-08
上传时间:	2013-07-09 15:04:29 (UTC+8)
出版者:	College Park: American Physical Society
摘要:	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.
關聯:	Physical Review D 80(4), 045021(11pages)
DOI:	10.1103/PhysRevD.80.045021
显示于类别:	[物理學系暨研究所] 期刊論文

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