Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4534
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dc.contributor.authorIyer, B.R.-
dc.contributor.authorKumar, Arvind-
dc.date.accessioned2012-05-25T08:15:36Z-
dc.date.available2012-05-25T08:15:36Z-
dc.date.issued1977-07-
dc.identifier.citationPramana, 1977, Vol. 8, p. 500-511.en
dc.identifier.issn0304-4289-
dc.identifier.issn0973-7111 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4534-
dc.descriptionOpen Accessen
dc.description.abstractThe weak-field low-velocity approximation of the Dirac equation in Kerr space-time is investigated. The interaction terms admit an interpretation in terms of a 'dipole-dipole' interaction in addition to spin coupling with the angular momentum of the rotating source. The gravitational gyrofactor for spin is identified. The charged case (Kerr-Newman) is studied using a minimal prescription for electromagnetic coupling in the locally inertial frame, and to the leading order the standard electromagnetic gyrofactor is retrieved. A first-order perturbation calculation of the shift of the Schwarzschild energy level yields the main interesting result of this work: anomalous Zeeman splitting of the energy level of a Dirac particle in the Kerr metric.en
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.relation.urihttp://dx.doi.org/10.1007/BF02872098en
dc.relation.urihttp://adsabs.harvard.edu/abs/1977Prama...8..500Ien
dc.rights1977, Springer Verlagen
dc.subjectblack holes (astronomy)en
dc.subjectcosmologyen
dc.subjectdirac equationen
dc.subjectspace-time functionsen
dc.subjectangular momentumen
dc.subjectastronomical modelsen
dc.subjectelectromagnetic couplingen
dc.subjectgravitational fieldsen
dc.subjectkerr effectsen
dc.subjectperturbation theoryen
dc.subjectzeeman effecten
dc.titleDirac equation in Kerr space-timeen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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