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Galileon inflation

Galileon inflation is a radiatively stable higher derivative model of inflation. The model is determined by a finite number of relevant operators which are protected by a covariant generalization of the Galileon shift symmetry. We show that the nongaussianity of the primordial density perturbation generated during an epoch of Galileon inflation is a particularly powerful observational probe of these models and that, when the speed of sound is small, fNL can be larger than the usual result fNL ~ 1/c_s^2.

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Co-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipAuthorshipAuthorshipAuthorshipAuthorshipTopic signalTopic signalTopic signalRelated contextWGalileon inflationpreprint / 2011AClare BurrageResearcherAClaudia de RhamResearcherADavid SeeryResearcherAAndrew J. TolleyResearcherTastro-ph.CO6979 worksTgr-qc10727 worksThep-th13268 works
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Galileon inflation

preprint / 2011

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