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Energy conditions in non-Riemannian spacetimes
dc.contributor.authorSmalley, Larry L.en_US
dc.contributor.authorKrisch, Jean P.en_US
dc.date.accessioned2006-04-10T17:42:15Z
dc.date.available2006-04-10T17:42:15Z
dc.date.issued1994-12-19en_US
dc.identifier.citationSmalley, Larry L., Krisch, Jean P. (1994/12/19)."Energy conditions in non-Riemannian spacetimes." Physics Letters A 196(1-2): 147-153. <http://hdl.handle.net/2027.42/31132>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6TVM-46X9RBF-W2/2/954ffc1d9ca0059fee9bfdfc6bfb78f5en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/31132
dc.description.abstractWe interpret the energy conditions in non-Riemannian spacetimes by applying them to a family of stationary, axially symmetric solutions for the gravitational field equations for an Einstein-Cartan theory in a Riemann-Cartan spacetime.en_US
dc.format.extent344320 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleEnergy conditions in non-Riemannian spacetimesen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbsecondlevelMathematicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Physics, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherDepartment of Physics, University of Alabama in Huntsville, Huntsville, AL 35899, USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/31132/1/0000029.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0375-9601(94)91062-6en_US
dc.identifier.sourcePhysics Letters Aen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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