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A space–time in toroidal coordinates

dc.contributor.authorKrisch, Jean P.en_US
dc.contributor.authorGlass, E. N.en_US
dc.date.accessioned2010-05-06T23:06:22Z
dc.date.available2010-05-06T23:06:22Z
dc.date.issued2003-07en_US
dc.identifier.citationKrisch, J. P.; Glass, E. N. (2003). "A space–time in toroidal coordinates." Journal of Mathematical Physics 44(7): 3046-3058. <http://hdl.handle.net/2027.42/71037>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/71037
dc.description.abstractWe present an exact solution of Einstein’s field equations in toroidal coordinates. The solution has three regions: an interior with a string equation of state; an Israel boundary layer; and an exterior with constant isotropic pressure and constant density, locally isometric to anti–de Sitter space–time. The exterior can be a cosmological vacuum with negative cosmological constant. The size and mass of the toroidal loop depend on the size of Λ. © 2003 American Institute of Physics.en_US
dc.format.extent3102 bytes
dc.format.extent101515 bytes
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dc.format.mimetypeapplication/pdf
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleA space–time in toroidal coordinatesen_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, Michgan 48109en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/71037/2/JMAPAQ-44-7-3046-1.pdf
dc.identifier.doi10.1063/1.1580999en_US
dc.identifier.sourceJournal of Mathematical Physicsen_US
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dc.owningcollnamePhysics, Department of


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