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dc.contributor.author Das, Saurya
dc.contributor.author Mukhopadhyay, Himan
dc.contributor.author Ramadevi, P.
dc.date.accessioned 2015-12-16T20:55:10Z
dc.date.available 2015-12-16T20:55:10Z
dc.date.issued 2015-12-16
dc.identifier.citation Das, S., Mukhopadhyay, H., & Ramadevi, P. (2005). The spectrum of rotating black holes and its implications for Hawking radiation. Classical and Quantum Gravity, 22(2), 453-465. https://doi.org/10.1088/0264-9381/22/2/015
dc.identifier.uri https://hdl.handle.net/10133/3837
dc.description Sherpa Romeo green journal. “This is an author-created, un-copyedited version of an article accepted for publication/published in Classical and Quantum Gravity. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it.” en_US
dc.description.abstract The reduced phase space formalism for quantising 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. en_US
dc.language.iso en_CA en_US
dc.subject Black holes en_US
dc.subject Rotating black holes en_US
dc.subject BTZ black hole en_US
dc.subject Kerr black hole en_US
dc.subject Hawking radiation en_US
dc.title Spectrum of rotating black holes and its implications for Hawking radiation en_US
dc.type Article en_US
dc.publisher.faculty Arts and Science en_US
dc.publisher.department Department of Physics en_US
dc.description.peer-review No en_US
dc.publisher.institution University of Lethbridge en_US
dc.publisher.institution Indian Institute of Technology en_US
dc.publisher.doi 10.1088/0264-9381/22/2/015


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