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Inflation and de Sitter holography
dc.contributor.authorLarsen, Finnen_US
dc.contributor.authorMcNees, Roberten_US
dc.date.accessioned2006-12-19T19:17:48Z
dc.date.available2006-12-19T19:17:48Z
dc.date.issued2003-07-01en_US
dc.identifier.citationLarsen, Finn; McNees, Robert (2003). "Inflation and de Sitter holography." Journal of High Energy Physics. 07(051). <http://hdl.handle.net/2027.42/49140>en_US
dc.identifier.issn1126-6708en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49140
dc.description.abstractWe develop the relation between de Sitter holography and inflation in detail with particular attention to cosmic density perturbations. We set up the Hamilton-Jacobi formalism to present a systematic treatment of the logarithmic corrections to a scale invariant spectrum. Our computations can be interpreted without reference to holography, as strong infra-red effects in gravity. This point of view may be relevant for the fine-tuning problems inherent to inflation.en_US
dc.format.extent3118 bytes
dc.format.extent369710 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleInflation and de Sitter holographyen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumMichigan Center for Theoretical Physics, University of Michigan, Ann Arbor, MI-48109, USAen_US
dc.contributor.affiliationumMichigan Center for Theoretical Physics, University of Michigan, Ann Arbor, MI-48109, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/49140/2/jhep072003051.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/1126-6708/2003/07/051en_US
dc.identifier.sourceJournal of High Energy Physics.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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