DC Field | Value | Language |
---|---|---|
dc.contributor.author | Park, WI | ko |
dc.contributor.author | Stewart, Ewan D | ko |
dc.date.accessioned | 2013-03-07T08:36:43Z | - |
dc.date.available | 2013-03-07T08:36:43Z | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.issued | 2008-01 | - |
dc.identifier.citation | PHYSICAL REVIEW D, v.77 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.uri | http://hdl.handle.net/10203/89805 | - |
dc.description.abstract | We analyze how the spectrum of perturbations produced in a multicomponent modular inflation model proposed by Kadota and Stewart depends on couplings between the two moduli. Although some simple direct couplings give essentially the same results as the original model, dn/dlnk proportional to n-1, simple indirect couplings produce a power law spectrum, n-1=constant, which can naturally be close to scale invariant. | - |
dc.language | English | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.subject | COSMOLOGICAL IMPLICATIONS | - |
dc.subject | PERTURBATIONS | - |
dc.subject | SUPERSYMMETRY | - |
dc.subject | BREAKING | - |
dc.subject | FIELD | - |
dc.title | Couplings and spectra in modular inflation | - |
dc.type | Article | - |
dc.identifier.wosid | 000252864000050 | - |
dc.identifier.scopusid | 2-s2.0-38849089326 | - |
dc.type.rims | ART | - |
dc.citation.volume | 77 | - |
dc.citation.publicationname | PHYSICAL REVIEW D | - |
dc.identifier.doi | 10.1103/PhysRevD.77.023535 | - |
dc.contributor.localauthor | Stewart, Ewan D | - |
dc.contributor.nonIdAuthor | Park, WI | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | COSMOLOGICAL IMPLICATIONS | - |
dc.subject.keywordPlus | PERTURBATIONS | - |
dc.subject.keywordPlus | SUPERSYMMETRY | - |
dc.subject.keywordPlus | BREAKING | - |
dc.subject.keywordPlus | FIELD | - |
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