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dc.contributor.authorIyer, B.R.-
dc.contributor.authorKumar, Arvind-
dc.date.accessioned2012-05-25T08:17:08Z-
dc.date.available2012-05-25T08:17:08Z-
dc.date.issued1979-02-
dc.identifier.citationPramana, 1979, Vol. 12, p103en
dc.identifier.issn0304-4289-
dc.identifier.issn0973-7111 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4536-
dc.descriptionOpen Accessen
dc.description.abstractUnruh's technique of replacing collapse by boundary conditions on the past horizon (the xi-quantization scheme) for the derivation of the well-known Hawking radiation is extended to the Kerr black hole for the scalar and especially for the spin half field. The expectation value of the energy momentum tensor is evaluated asymptotically in the xi-vacuum state yielding explicitly the net Hawking flux of scalar and spin half quanta. The appropriate statistical distribution that emerges naturally for Dirac quanta validates the xi-scheme for fermions and confirms the association of temperature with a Kerr black hole.en
dc.language.isoenen
dc.publisherSpringer Verlagen
dc.relation.urihttp://dx.doi.org/ 10.1007/BF02846113en
dc.relation.urihttp://adsabs.harvard.edu/abs/1979Prama..12..103Ien
dc.rights1979, Springer Verlagen
dc.subjectblack holes (astronomy)en
dc.subjectfermi-dirac statisticsen
dc.subjectfermionsen
dc.subjectquantum statisticsen
dc.subjectscalarsen
dc.subjectspin dynamicsen
dc.subjectangular momentumen
dc.subjecteuler-lagrange equationen
dc.subjectstatistical distributionsen
dc.subjectstellar massen
dc.subjectstellar radiationen
dc.subjecttensor analysisen
dc.titleHawking radiation of scalar and Dirac quanta from a Kerr black holeen
dc.typeArticleen
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