Journal
JOURNAL OF MATHEMATICAL PHYSICS
Volume 55, Issue 11, Pages -Publisher
AMER INST PHYSICS
DOI: 10.1063/1.4901127
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Funding
- Ratchadapisek Sompoch Endowment Fund, Chulalongkorn University [Sci-Super 2014-032]
- Thailand Toray Science Foundation (TTSF)
- Thailand Research Fund (TRF)
- Office of the Higher Education Commission (OHEC), Faculty of Science, Chulalongkorn University [MRG5680171]
- Research Strategic plan program [A1B1]
- Thailand Excellence in Physics project (THEP)
- Royal Government of Thailand
- Development and Promotion of Science and Technology talent project (DPST)
- Marsden Fund
- James Cook fellowship
- Ratchadapisek Somphot Fund at Chulalongkorn University
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The Myers-Perry black holes are higher-dimensional generalizations of the usual (3 + 1)-dimensional rotating Kerr black hole. They are of considerable interest in Kaluza-Klein models, specifically within the context of brane-world versions thereof. In the present article, we shall consider the greybody factors associated with scalar field excitations of the Myers-Perry spacetimes, and develop some rigorous bounds on these greybody factors. These bounds are of relevance for characterizing both the higher-dimensional Hawking radiation, and the super-radiance, that is expected for these spacetimes. (C) 2014 AIPPublishing LLC.
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