Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/7654
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dc.contributorDepartment of Applied Mathematics-
dc.creatorLun, AWC-
dc.date.accessioned2015-11-10T08:33:02Z-
dc.date.available2015-11-10T08:33:02Z-
dc.identifier.issn0022-2488 (print)-
dc.identifier.issn1089-7658 (online)-
dc.identifier.urihttp://hdl.handle.net/10397/7654-
dc.language.isoenen_US
dc.publisherAmerican Institute of Physicsen_US
dc.rights© 1980 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in Anthony W.C. Lun, J. Math. Phys., 21, 2257 (1980) and may be found at http://link.aip.org/link/?jmp/21/2257en_US
dc.subjectNeutrino-gravitational solutionsen_US
dc.titleKerr-like neutrino-gravitational solutionsen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.spage2257-
dc.identifier.epage2260-
dc.identifier.volume21-
dc.identifier.issue8-
dc.identifier.doi10.1063/1.524662-
dcterms.abstractTwo distinct stationary axisymmetric Kerr‐like neutrino‐gravitational space–times are presented. They reduce to the Kerr solution when the neutrino field vanishes. In addition, the first solution possesses physical line singularities along the axis of symmetry; whereas the second solution is asymptotically flat and its locally bounded Riemann tensor is discontinuous at the equatorial plane. Both metrics are of Petrov type II and their neutrino fields belong to type [2N‐2S]₍₂₋₁₎ in the Plebański classification.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationJournal of mathematical physics, Aug. 1980, v. 21, no. 8, p. 2257-2260-
dcterms.isPartOfJournal of mathematical physics-
dcterms.issued1980-08-
dc.identifier.isiWOS:A1980KC80600037-
dc.identifier.scopus2-s2.0-36749104577-
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_IR/PIRAen_US
dc.description.pubStatusPublisheden_US
dc.description.oaCategoryVoR alloweden_US
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