DC Field | Value | Language |
---|---|---|
dc.contributor.author | Lyth, DH | ko |
dc.contributor.author | Stewart, Ewan D | ko |
dc.date.accessioned | 2013-03-02T22:15:29Z | - |
dc.date.available | 2013-03-02T22:15:29Z | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.issued | 1996-02 | - |
dc.identifier.citation | PHYSICAL REVIEW D, v.53, no.4, pp.1784 - 1798 | - |
dc.identifier.issn | 0556-2821 | - |
dc.identifier.uri | http://hdl.handle.net/10203/75816 | - |
dc.description.abstract | In supersymmetric theories a field can develop a vacuum expectation value M much greater than 10(3) GeV, even though its mass m is of order 10(2) to 10(3) GeV. The finite temperature in the early Universe can hold such a field at zero, corresponding to a false vacuum with energy density V-0 similar to m(2) M(2). When the temperature falls below V-0(1/4), the thermal energy density becomes negligible and an era of thermal inflation begins. It ends when the field rolls away from zero at a temperature of order m, corresponding to of order 10 e-folds of inflation which does not affect the density perturbation generated during ordinary inflation. Thermal inflation can solve the Polonyi/moduli problem if M is within one or two orders of magnitude of 10(12) GeV. | - |
dc.language | English | - |
dc.publisher | AMERICAN PHYSICAL SOC | - |
dc.subject | SUPERSTRING MODELS | - |
dc.subject | PHASE-TRANSITIONS | - |
dc.subject | PARTICLE PHYSICS | - |
dc.subject | COSMOLOGICAL PROBLEMS | - |
dc.subject | SYMMETRY-BREAKING | - |
dc.subject | NATURAL INFLATION | - |
dc.subject | GRAVITINO PROBLEM | - |
dc.subject | ENTROPY CRISIS | - |
dc.subject | SCALE | - |
dc.subject | AXIONS | - |
dc.title | Thermal inflation and the moduli problem | - |
dc.type | Article | - |
dc.identifier.wosid | A1996TW98200009 | - |
dc.identifier.scopusid | 2-s2.0-12844280357 | - |
dc.type.rims | ART | - |
dc.citation.volume | 53 | - |
dc.citation.issue | 4 | - |
dc.citation.beginningpage | 1784 | - |
dc.citation.endingpage | 1798 | - |
dc.citation.publicationname | PHYSICAL REVIEW D | - |
dc.identifier.doi | 10.1103/PhysRevD.53.1784 | - |
dc.contributor.localauthor | Stewart, Ewan D | - |
dc.contributor.nonIdAuthor | Lyth, DH | - |
dc.description.isOpenAccess | N | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | SUPERSTRING MODELS | - |
dc.subject.keywordPlus | PHASE-TRANSITIONS | - |
dc.subject.keywordPlus | PARTICLE PHYSICS | - |
dc.subject.keywordPlus | COSMOLOGICAL PROBLEMS | - |
dc.subject.keywordPlus | SYMMETRY-BREAKING | - |
dc.subject.keywordPlus | NATURAL INFLATION | - |
dc.subject.keywordPlus | GRAVITINO PROBLEM | - |
dc.subject.keywordPlus | ENTROPY CRISIS | - |
dc.subject.keywordPlus | SCALE | - |
dc.subject.keywordPlus | AXIONS | - |
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