The density perturbation power spectrum to second-order corrections in the slow-roll expansion
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Stewart, Ewan D | ko |
| dc.contributor.author | Gong, JO | ko |
| dc.date.accessioned | 2013-03-03T10:56:34Z | - |
| dc.date.available | 2013-03-03T10:56:34Z | - |
| dc.date.created | 2012-02-06 | - |
| dc.date.created | 2012-02-06 | - |
| dc.date.issued | 2001-06 | - |
| dc.identifier.citation | PHYSICS LETTERS B, v.510, no.1-4, pp.1 - 9 | - |
| dc.identifier.issn | 0370-2693 | - |
| dc.identifier.uri | http://hdl.handle.net/10203/78414 | - |
| dc.description.abstract | We set up a formalism that can be used to calculate the power spectrum of the curvature perturbations produced during inflation up to arbitrary order in the slow-roll expansion, and explicitly calculate the power spectrum and spectral index up to second-order corrections. (C) 2001 Elsevier Science B.V. All rights reserved. | - |
| dc.language | English | - |
| dc.publisher | ELSEVIER SCIENCE BV | - |
| dc.subject | COSMOLOGICAL PERTURBATIONS | - |
| dc.subject | INFLATIONARY PERTURBATIONS | - |
| dc.subject | APPROXIMATION | - |
| dc.subject | UNIVERSE | - |
| dc.title | The density perturbation power spectrum to second-order corrections in the slow-roll expansion | - |
| dc.type | Article | - |
| dc.identifier.wosid | 000169542300001 | - |
| dc.identifier.scopusid | 2-s2.0-0001909512 | - |
| dc.type.rims | ART | - |
| dc.citation.volume | 510 | - |
| dc.citation.issue | 1-4 | - |
| dc.citation.beginningpage | 1 | - |
| dc.citation.endingpage | 9 | - |
| dc.citation.publicationname | PHYSICS LETTERS B | - |
| dc.contributor.localauthor | Stewart, Ewan D | - |
| dc.contributor.nonIdAuthor | Gong, JO | - |
| dc.type.journalArticle | Article | - |
| dc.subject.keywordPlus | COSMOLOGICAL PERTURBATIONS | - |
| dc.subject.keywordPlus | INFLATIONARY PERTURBATIONS | - |
| dc.subject.keywordPlus | APPROXIMATION | - |
| dc.subject.keywordPlus | UNIVERSE | - |
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