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dc.contributor.authorRandall, Lisa
dc.contributor.authorSchwartz, Matthew D.
dc.contributor.authorThambyahpillai, Shiyamala
dc.date.accessioned2019-09-27T13:17:51Z
dc.date.issued2005
dc.identifier.citationRandall, Lisa, Matthew D Schwartz, and Shiyamala Thambyahpillai. 2005. “Discretizing Gravity in Warped Spacetime.” Journal of High Energy Physics 2005 (10): 110–110. https://doi.org/10.1088/1126-6708/2005/10/110.
dc.identifier.issn1029-8479
dc.identifier.issn1126-6708
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41417355*
dc.description.abstractWe investigate the discretized version of the compact Randall-Sundrum model. By studying the mass eigenstates of the lattice theory, we demonstrate that for warped space, unlike for flat space, the strong coupling scale does not depend on the IR scale and lattice size. However, strong coupling does prevent us from taking the continuum limit of the lattice theory. Nonetheless, the lattice theory works in the manifestly holographic regime and successfully reproduces the most significant features of the warped theory. It is even in some respects better than the KK theory, which must be carefully regulated to obtain the correct physical results. Because it is easier to construct lattice theories than to find exact solutions to GR, we expect lattice gravity to be a useful tool for exploring field theory in curved space.
dc.language.isoen_US
dc.publisherSpringer Verlag
dash.licenseLAA
dc.titleDiscretizing gravity in warped spacetime
dc.typeJournal Article
dc.description.versionVersion of Record
dc.relation.journalJournal of High Energy Physics
dash.depositing.authorRandall, Lisa::08d670e0eeaed6b678e474a11d0afaf0::600
dc.date.available2019-09-27T13:17:51Z
dash.workflow.comments1Science Serial ID 47492
dc.identifier.doi10.1088/1126-6708/2005/10/110
dash.source.volume2005;10
dash.source.page110-110


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