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Spinning up asymptotically flat spacetimes

dc.contributor.authorGlass, E. N.en_US
dc.contributor.authorKrisch, Jean P.en_US
dc.date.accessioned2006-12-19T19:23:49Z
dc.date.available2006-12-19T19:23:49Z
dc.date.issued2004-12-07en_US
dc.identifier.citationGlass, E N; Krisch, J P (2004). "Spinning up asymptotically flat spacetimes." Classical and Quantum Gravity. 21(23): 5543-5553. <http://hdl.handle.net/2027.42/49214>en_US
dc.identifier.issn0264-9381en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49214
dc.description.abstractWe present a method for constructing stationary, asymptotically flat, rotating solutions of Einstein's field equations. One of the spun-up solutions has quasilocal mass but no global mass. It has an ergosphere but no event horizon. The angular momentum is constant everywhere beyond the ergosphere. The energy–momentum content of this solution can be interpreted as a rotating string fluid.en_US
dc.format.extent3118 bytes
dc.format.extent136214 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleSpinning up asymptotically flat spacetimesen_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/2027.42/49214/2/cqg4_23_015.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/0264-9381/21/23/015en_US
dc.identifier.sourceClassical and Quantum Gravity.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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