Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1236
Full metadata record
DC FieldValueLanguage
dc.contributor.authorIyer, B.R.-
dc.contributor.authorVishveshwara, C.V.-
dc.date.accessioned2006-05-16T06:39:05Z-
dc.date.available2006-05-16T06:39:05Z-
dc.date.issued1985-05-
dc.identifier.citationJournal of Mathematical Physics, 1985, Vol.26, p1034-1039en
dc.identifier.issn0022-2488-
dc.identifier.urihttp://hdl.handle.net/2289/1236-
dc.description.abstractChandrasekhar's technique for separation of the Dirac equation in the Kerr background is applied to perfect fluid space-times with local rotational symmetry. These space-times fall into three distinct types. It is found that in case (1) the Dirac equation separates if the space-time is at least ``locally static'' while in case (3) it separates if the space-time is at least ``locally diagonal,'' in contrast to the massless case where Dhurandhar, Vishveshwara, and Cohen showed that the Hertz potential is separable in all cases. In case (2), however, the Dirac equation is separable in all those cases where the Hertz potential for neutrinos is separable.en
dc.format.extent322154 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Institute of Physicsen
dc.relation.urihttp://link.aip.org/link/?jmp/26/1034en
dc.rights(1985) 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.en
dc.titleSeparability of the Dirac equation in a class of perfect fluid space-times with local rotational symmetryen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

Files in This Item:
File Description SizeFormat 
1985 J Mat Phys V26 p1034.pdf6p.314.6 kBAdobe PDFView/Open


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.