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Spin fluid spacetimes from static general relativistic solutions

dc.contributor.authorKrisch, Jean P.en_US
dc.contributor.authorSmalley, Larry L.en_US
dc.date.accessioned2006-12-19T19:22:09Z
dc.date.available2006-12-19T19:22:09Z
dc.date.issued1993-05-01en_US
dc.identifier.citationKrisch, J P; Smalley, L L (1993). "Spin fluid spacetimes from static general relativistic solutions." Classical and Quantum Gravity. 10(5): 995-1003. <http://hdl.handle.net/2027.42/49193>en_US
dc.identifier.issn0264-9381en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49193
dc.description.abstractA method for generating spin fluid solutions to the field equations in a Riemann-Cartan spacetime is presented. The method uses any general relativistic static perfect fluid solution as input. The resulting RC solutions are irrotational and stationary. They will support a nonzero spin density. The spin density has zero Fermi derivative and will not contribute to a circulation.en_US
dc.format.extent3118 bytes
dc.format.extent365121 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleSpin fluid spacetimes from static general relativistic solutionsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationotherDept. of Phys., Michigan Univ., Ann Arbor, MI, USAen_US
dc.contributor.affiliationotherDept. of Phys., Michigan Univ., Ann Arbor, MI, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/49193/2/cq930516.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/0264-9381/10/5/016en_US
dc.identifier.sourceClassical and Quantum Gravity.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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