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The spectrum of rotating black holes and its implications for Hawking radiation

DSpace at IIT Bombay

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Title The spectrum of rotating black holes and its implications for Hawking radiation
 
Creator DAS, S
MUKHOPADHYAY, H
RAMADEVI, P
 
Subject quasi-normal modes
area spectrum
quantum-gravity
mass-spectrum
quantization
entropy
dimensions
millimeter
foam
tev
 
Description The reduced phase space formalism for quantizing black holes has recently been extended to find the area and angular momentum spectra of four-dimensional Kerr black holes. We extend this further to rotating black holes in all spacetime dimensions and show that although as in four dimensions the spectrum is discrete, it is not equispaced in general. As a result, Hawking radiation spectra from these black holes are continuous, as opposed to the discrete spectrum predicted for four-dimensional black holes.
 
Publisher IOP PUBLISHING LTD
 
Date 2011-08-04T01:50:42Z
2011-12-26T12:54:29Z
2011-12-27T05:42:26Z
2011-08-04T01:50:42Z
2011-12-26T12:54:29Z
2011-12-27T05:42:26Z
2005
 
Type Article
 
Identifier CLASSICAL AND QUANTUM GRAVITY, 22(2), 453-465
0264-9381
http://dx.doi.org/10.1088/0264-9381/22/2/015
http://dspace.library.iitb.ac.in/xmlui/handle/10054/9209
http://hdl.handle.net/10054/9209
 
Language en