DC Field | Value | Language |
---|---|---|
dc.contributor.author | Dodelson, S | ko |
dc.contributor.author | Kaplinghat, M | ko |
dc.contributor.author | Stewart, Ewan D | ko |
dc.date.accessioned | 2013-02-28T00:54:43Z | - |
dc.date.available | 2013-02-28T00:54:43Z | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.issued | 2000-12 | - |
dc.identifier.citation | PHYSICAL REVIEW LETTERS, v.85, no.25, pp.5276 - 5279 | - |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.uri | http://hdl.handle.net/10203/71856 | - |
dc.description.abstract | Recent cosmological observations strongly suggest that the Universe is dominated by an unknown form of energy with negative pressure. Why is this dark energy density of order the critical density today? We propose that the dark energy has periodically dominated in the past so that its preponderance toda; is natural. We illustrate this paradigm with a model potential and show that its predictions are consistent with all observations. | - |
dc.language | English | - |
dc.publisher | AMERICAN PHYSICAL SOC | - |
dc.subject | COLD DARK-MATTER | - |
dc.subject | MICROWAVE BACKGROUND ANISOTROPY | - |
dc.subject | COSMOLOGICAL CONSTANT | - |
dc.subject | UNIVERSE | - |
dc.subject | LAMBDA | - |
dc.subject | MODELS | - |
dc.subject | CONSTRAINTS | - |
dc.subject | STATE | - |
dc.subject | CONSEQUENCES | - |
dc.subject | PARAMETERS | - |
dc.title | Solving the coincidence problem: Tracking oscillating energy | - |
dc.type | Article | - |
dc.identifier.wosid | 000165884200004 | - |
dc.identifier.scopusid | 2-s2.0-0034506965 | - |
dc.type.rims | ART | - |
dc.citation.volume | 85 | - |
dc.citation.issue | 25 | - |
dc.citation.beginningpage | 5276 | - |
dc.citation.endingpage | 5279 | - |
dc.citation.publicationname | PHYSICAL REVIEW LETTERS | - |
dc.contributor.localauthor | Stewart, Ewan D | - |
dc.contributor.nonIdAuthor | Dodelson, S | - |
dc.contributor.nonIdAuthor | Kaplinghat, M | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | COLD DARK-MATTER | - |
dc.subject.keywordPlus | MICROWAVE BACKGROUND ANISOTROPY | - |
dc.subject.keywordPlus | COSMOLOGICAL CONSTANT | - |
dc.subject.keywordPlus | UNIVERSE | - |
dc.subject.keywordPlus | LAMBDA | - |
dc.subject.keywordPlus | MODELS | - |
dc.subject.keywordPlus | CONSTRAINTS | - |
dc.subject.keywordPlus | STATE | - |
dc.subject.keywordPlus | CONSEQUENCES | - |
dc.subject.keywordPlus | PARAMETERS | - |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.