Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4531
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dc.contributor.authorIyer, B.R.-
dc.contributor.authorKumar, Arvind-
dc.date.accessioned2012-05-24T04:29:06Z-
dc.date.available2012-05-24T04:29:06Z-
dc.date.issued1978-12-19-
dc.identifier.citationJournal of Physics A - Mathematical and General, 1979, Vol.12, p1795-1803en
dc.identifier.issn1751-8113-
dc.identifier.issn1751-8121 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/4531-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstracthe v vacuum discussed recently by Fulling (1977) in his general study of alternative vacuum states in space-times with horizons is investigated specifically for the scalar and Dirac fields in Kerr space-time. An explicit evaluation of flux shows that except for the effects due to super-radiance of scalar waves, this vacuum corresponds to a black hole in thermal equilibrium with its environment.en
dc.language.isoenen
dc.publishernstitute of Physicsen
dc.relation.urihttp://dx.doi.org/ 10.1088/0305-4470/12/10/025en
dc.relation.urihttp://adsabs.harvard.edu/abs/1979JPhA...12.1795Ien
dc.rights1979, Institute of Physicsen
dc.subjectblack holes (astronomy)en
dc.subjectthermodynamic equilibriumen
dc.subjectvacuumen
dc.subjectastrophysicsen
dc.subjectasymptotic methodsen
dc.subjectchandrasekhar equationen
dc.subjectdirac equationen
dc.subjectscalarsen
dc.subjectspace-time functionsen
dc.titleThe Kerr black hole in thermal equilibrium and the V vacuumen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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