Gravitational waves from warped spacetime
Author
Randall, Lisa
Servant, Géraldine
Published Version
https://doi.org/10.1088/1126-6708/2007/05/054Metadata
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Randall, 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.Abstract
We 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.Terms of Use
This article is made available under the terms and conditions applicable to Other Posted Material, as set forth at http://nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of-use#LAACitable link to this page
http://nrs.harvard.edu/urn-3:HUL.InstRepos:41417363
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