A new delta N formalism for multi-component inflation

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dc.contributor.authorLee, HCko
dc.contributor.authorSasaki, Mko
dc.contributor.authorStewart, Ewan Dko
dc.contributor.authorTanaka, Tko
dc.contributor.authorYokoyama, Sko
dc.date.accessioned2013-03-07T21:03:58Z-
dc.date.available2013-03-07T21:03:58Z-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.issued2005-10-
dc.identifier.citationJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, v.53, pp.3415 - 3421-
dc.identifier.issn1475-7516-
dc.identifier.urihttp://hdl.handle.net/10203/91316-
dc.description.abstractThe delta N formula that relates the. final curvature perturbation on comoving slices to the in. inflaton perturbation on. at slices after horizon crossing is a powerful and intuitive tool for computing the curvature perturbation spectrum from inflation. However, it is customarily assumed further that the conventional slow-roll condition is satisfied, and satisfied by all components, during horizon crossing. In this paper, we develop a new dN formalism for multi-component inflation that can be applied in the most general situations. This allows us to generalize the idea of general slow-roll inflation to the multi-component case, in particular only applying the general slow-roll condition to the relevant component. We compute the power spectrum of the curvature perturbation in multi-component general slow-roll inflation, and find that under quite general conditions it is invertible.-
dc.languageEnglish-
dc.publisherIOP PUBLISHING LTD-
dc.subjectPERTURBATIONS-
dc.subject2ND-ORDER-
dc.subjectSPECTRUM-
dc.titleA new delta N formalism for multi-component inflation-
dc.typeArticle-
dc.identifier.wosid000233122400014-
dc.identifier.scopusid2-s2.0-27744464529-
dc.type.rimsART-
dc.citation.volume53-
dc.citation.beginningpage3415-
dc.citation.endingpage3421-
dc.citation.publicationnameJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS-
dc.identifier.doi10.1088/1475-7516/2005/10/004-
dc.contributor.localauthorStewart, Ewan D-
dc.contributor.nonIdAuthorLee, HC-
dc.contributor.nonIdAuthorSasaki, M-
dc.contributor.nonIdAuthorTanaka, T-
dc.contributor.nonIdAuthorYokoyama, S-
dc.type.journalArticleArticle-
dc.subject.keywordAuthorcosmological perturbation theory-
dc.subject.keywordAuthorinflation-
dc.subject.keywordAuthorphysics of the early universe-
dc.subject.keywordPlusPERTURBATIONS-
dc.subject.keywordPlus2ND-ORDER-
dc.subject.keywordPlusSPECTRUM-
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