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Two-fluid atmosphere for relativistic stars
dc.contributor.authorGlass, E. N.en_US
dc.contributor.authorKrisch, Jean P.en_US
dc.date.accessioned2006-12-19T19:22:47Z
dc.date.available2006-12-19T19:22:47Z
dc.date.issued1999-04-01en_US
dc.identifier.citationGlass, E N; Krisch, J P (1999). "Two-fluid atmosphere for relativistic stars ." Classical and Quantum Gravity. 16(4): 1175-1184. <http://hdl.handle.net/2027.42/49201>en_US
dc.identifier.issn0264-9381en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49201
dc.description.abstractWe have extended the Vaidya radiating metric to include both a radiation fluid and a string fluid. This paper expands our brief introduction to extensions of the Schwarzschild vacuum which appeared in 1998 Phys. Rev. D 57 R5945. Assuming diffusive transport for the string fluid, we find new analytic solutions of Einstein's field equations.en_US
dc.format.extent3118 bytes
dc.format.extent134922 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleTwo-fluid atmosphere for relativistic starsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_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.affiliationumDepartment of Physics, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/49201/2/q90407.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/0264-9381/16/4/007en_US
dc.identifier.sourceClassical and Quantum Gravity.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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