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Exact solutions for space-times with local rotational symmetry in which the Dirac equation separates

dc.contributor.authorIyer, B R
dc.contributor.authorVishveshwara, C V
dc.date.accessioned2006-05-16T09:18:48Z
dc.date.available2006-05-16T09:18:48Z
dc.date.issued1987-06
dc.description.abstractThe field equations for the class of perfect fluid space-times with local rotational symmetry which the authors had earlier shown the Dirac equation separates are studied. For the vacuum and dust cases all possible solutions are exhibited. Other solutions correspond to radiation, a stiff fluid, and a fluid with negative pressure.en
dc.format.extent241119 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationJournal of Mathematical Physics, 1987, Vol.28, p1377-1381en
dc.identifier.issn0022-2488
dc.identifier.urihttp://hdl.handle.net/2289/1242
dc.language.isoenen
dc.publisherThe American Institute of Physicsen
dc.relation.urihttp://link.aip.org/link/?jmp/28/1377en
dc.rights(1987) 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.titleExact solutions for space-times with local rotational symmetry in which the Dirac equation separatesen
dc.typeArticleen

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