Non-abelian discrete gauge symmetries and inflation

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dc.contributor.authorCohn, JDko
dc.contributor.authorStewart, Ewan Dko
dc.date.accessioned2013-02-27T10:56:52Z-
dc.date.available2013-02-27T10:56:52Z-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.issued2000-03-
dc.identifier.citationPHYSICS LETTERS B, v.475, no.3-4, pp.231 - 235-
dc.identifier.issn0370-2693-
dc.identifier.urihttp://hdl.handle.net/10203/68099-
dc.description.abstractObtaining a potential flat enough to provide slow roll inflation is often difficult when gravitational effects are included. Non-abelian discrete gauge symmetries can guarantee the flatness of the inflaton potential in this case, and also provide special field values where inflation can end. (C) 2000 Elsevier Science B.V. All rights reserved.-
dc.languageEnglish-
dc.publisherELSEVIER SCIENCE BV-
dc.subjectLARGE-SCALE STRUCTURE-
dc.subjectHYBRID INFLATION-
dc.subjectDENSITY PERTURBATIONS-
dc.subjectNATURAL INFLATION-
dc.subjectENTROPY CRISIS-
dc.subjectSUPERSYMMETRY-
dc.subjectSUPERGRAVITY-
dc.titleNon-abelian discrete gauge symmetries and inflation-
dc.typeArticle-
dc.identifier.wosid000085735100005-
dc.identifier.scopusid2-s2.0-0034594847-
dc.type.rimsART-
dc.citation.volume475-
dc.citation.issue3-4-
dc.citation.beginningpage231-
dc.citation.endingpage235-
dc.citation.publicationnamePHYSICS LETTERS B-
dc.contributor.localauthorStewart, Ewan D-
dc.contributor.nonIdAuthorCohn, JD-
dc.type.journalArticleArticle-
dc.subject.keywordPlusLARGE-SCALE STRUCTURE-
dc.subject.keywordPlusHYBRID INFLATION-
dc.subject.keywordPlusDENSITY PERTURBATIONS-
dc.subject.keywordPlusNATURAL INFLATION-
dc.subject.keywordPlusENTROPY CRISIS-
dc.subject.keywordPlusSUPERSYMMETRY-
dc.subject.keywordPlusSUPERGRAVITY-
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