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dc.contributor.authorRandall, Lisa
dc.contributor.authorServant, Géraldine
dc.date.accessioned2019-09-27T13:18:11Z
dc.date.issued2007
dc.identifier.citationRandall, Lisa, and Géraldine Servant. 2007. “Gravitational Waves from Warped Spacetime.” Journal of High Energy Physics 2007 (5): 054–054. https://doi.org/10.1088/1126-6708/2007/05/054.
dc.identifier.issn1029-8479
dc.identifier.issn1126-6708
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41417363*
dc.description.abstractWe argue that the RSI model can provide a strong signature in a gravitational waves. This signal is a relic stochastic background generated during the cosmological phase transition from an AdS-Schwarschild phase to the RS1 geometry that should occur at a temperature in the TeV range. We estimate the amplitude of the signal in terms of the parameters of the potential stabilizing the radion and show that over much of the parameter region in which the phase transition completes, a signal should be detectable at the planned space interferometer, LISA.
dc.language.isoen_US
dc.publisherSpringer Verlag
dash.licenseLAA
dc.titleGravitational waves from 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.available2019-09-27T13:18:11Z
dash.workflow.comments1Science Serial ID 47542
dc.identifier.doi10.1088/1126-6708/2007/05/054
dash.source.volume2007;5
dash.source.page54


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