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dc.contributor.author Das, Saurya
dc.contributor.author Robinson, Sean P.
dc.contributor.author Vagenas, Elias C.
dc.date.accessioned 2016-01-07T21:23:19Z
dc.date.available 2016-01-07T21:23:19Z
dc.date.issued 2016-01-07
dc.identifier.citation Das, S., Robinson, S. P., & Vagenas, E. C. (2008). Gravitational anaomalies: A recipe for Hawking radiation. International Journal of Modern Physics D, 17(03-04), 533-539. https://doi.org/10.1142/S0218271808012218
dc.identifier.uri https://hdl.handle.net/10133/3860
dc.description Sherpa Romeo yellow journal. Preprint of an article published in International Journal of Modern Physics D © World Scientific Publishing Company https://www.worldscientific.com/worldscinet/ijmpd en_US
dc.description.abstract We explore the method of Robinson andWilczek for deriving the Hawking temperature of a black hole. In this method, the Hawking radiation restores general covariance in an effective theory of near-horizon physics which otherwise exhibits a gravitational anomaly at the quantum level. The method has been shown to work for broad classes of black holes in arbitrary spacetime dimensions. These include static black holes, accreting or evaporating black holes, charged black holes, rotating black holes, and even black rings. In the cases of charged and rotating black holes, the expected super-radiant current is also reproduced. en_US
dc.language.iso en_CA en_US
dc.subject Hawking temperature en_US
dc.subject Gravitational anomaly en_US
dc.subject Black holes en_US
dc.subject Hawking radiation en_US
dc.title Gravitational anomalies: a recipe 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 Massachusetts Institute of Technology en_US
dc.publisher.institution University of Athens en_US


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