DC Field | Value | Language |
---|---|---|
dc.contributor.author | Stewart, Ewan D | ko |
dc.date.accessioned | 2013-02-28T02:45:35Z | - |
dc.date.available | 2013-02-28T02:45:35Z | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.issued | 1997-01 | - |
dc.identifier.citation | PHYSICS LETTERS B, v.391, no.1-2, pp.34 - 38 | - |
dc.identifier.issn | 0370-2693 | - |
dc.identifier.uri | http://hdl.handle.net/10203/72360 | - |
dc.description.abstract | I show that a classical scalar potential with V ''/V similar to 1 can be sufficiently flattened by quantum corrections to give rise to slow roll inflation. This provides perhaps the simplest way to generate an inflationary potential without fine-tuning. The most natural implementation of this idea produces an unviably small spectral index, but, for example, n similar to 0.8 can be obtained in other implementations. | - |
dc.language | English | - |
dc.publisher | ELSEVIER SCIENCE BV | - |
dc.subject | NATURAL INFLATION | - |
dc.subject | PARTICLE PHYSICS | - |
dc.subject | SUPERGRAVITY | - |
dc.title | Flattening the inflatons potential with quantum corrections | - |
dc.type | Article | - |
dc.identifier.wosid | A1997WD16700007 | - |
dc.identifier.scopusid | 2-s2.0-0041593664 | - |
dc.type.rims | ART | - |
dc.citation.volume | 391 | - |
dc.citation.issue | 1-2 | - |
dc.citation.beginningpage | 34 | - |
dc.citation.endingpage | 38 | - |
dc.citation.publicationname | PHYSICS LETTERS B | - |
dc.identifier.doi | 10.1016/S0370-2693(96)01458-X | - |
dc.contributor.localauthor | Stewart, Ewan D | - |
dc.description.isOpenAccess | N | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | NATURAL INFLATION | - |
dc.subject.keywordPlus | PARTICLE PHYSICS | - |
dc.subject.keywordPlus | SUPERGRAVITY | - |
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