MUTATED HYBRID INFLATION
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Stewart, Ewan D | ko |
| dc.date.accessioned | 2013-02-27T21:26:14Z | - |
| dc.date.available | 2013-02-27T21:26:14Z | - |
| dc.date.created | 2012-02-06 | - |
| dc.date.created | 2012-02-06 | - |
| dc.date.issued | 1995-02 | - |
| dc.identifier.citation | PHYSICS LETTERS B, v.345, no.4, pp.414 - 415 | - |
| dc.identifier.issn | 0370-2693 | - |
| dc.identifier.uri | http://hdl.handle.net/10203/70939 | - |
| dc.description.abstract | A new model of inflation is described. An unusual form for the inflationary potential is obtained because the inflaton corresponds to a non-trivial path in the configuration space of the two real scalar fields of the model. The model predicts a spectral index n = 1 - 3/2N similar or equal to 0.97 for the density perturbations and negligible gravitational waves. | - |
| dc.language | English | - |
| dc.publisher | ELSEVIER SCIENCE BV | - |
| dc.title | MUTATED HYBRID INFLATION | - |
| dc.type | Article | - |
| dc.identifier.wosid | A1995QJ71100013 | - |
| dc.identifier.scopusid | 2-s2.0-0001569813 | - |
| dc.type.rims | ART | - |
| dc.citation.volume | 345 | - |
| dc.citation.issue | 4 | - |
| dc.citation.beginningpage | 414 | - |
| dc.citation.endingpage | 415 | - |
| dc.citation.publicationname | PHYSICS LETTERS B | - |
| dc.identifier.doi | 10.1016/0370-2693(94)01646-T | - |
| dc.contributor.localauthor | Stewart, Ewan D | - |
| dc.description.isOpenAccess | N | - |
| dc.type.journalArticle | Article | - |
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