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Quasi-Single Field Inflation with Large Mass

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arxiv 1205.0160 v2 pith:JMMTVVNW submitted 2012-05-01 hep-th astro-ph.COgr-qchep-ph

Quasi-Single Field Inflation with Large Mass

classification hep-th astro-ph.COgr-qchep-ph
keywords massordercorrectionfieldinflationisocurvatonlargequasi-single
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the effect of massive isocurvaton on density perturbations in quasi-single field inflation models, when the mass of the isocurvaton M becomes larger than the order of the Hubble parameter H. We analytically compute the correction to the power spectrum, leading order in coupling but exact for all values of mass. This verifies the previous numerical results for the range 0<M<3H/2 and shows that, in the large mass limit, the correction is of order H^2/M^2.

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Cited by 15 Pith papers

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