dc.contributor.author | Grøn, Øyvind | |
dc.date.accessioned | 2023-01-30T09:52:36Z | |
dc.date.available | 2023-01-30T09:52:36Z | |
dc.date.created | 2022-10-10T08:32:17Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Universe. 2022, 8 (9), . | en_US |
dc.identifier.issn | 2218-1997 | |
dc.identifier.uri | https://hdl.handle.net/11250/3047022 | |
dc.description.abstract | More than 30 inflationary models are confronted with the recently improved limit on the tensor-to-scalar ratio presented by the Planck team. I show that a few more models are falsified due to this sharper restriction. Additionally, I discuss possible consequences of CMB-S4 observations for these inflationary models. The results are summarized in a table. | en_US |
dc.language.iso | eng | en_US |
dc.rights | Navngivelse 4.0 Internasjonal | * |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/deed.no | * |
dc.title | Consequences of the improved limits on the tnsor-to-scalar ratio from BICEP/Planck, and of future CMB-S4 measurements, for inflationary models | en_US |
dc.type | Peer reviewed | en_US |
dc.type | Journal article | en_US |
dc.description.version | publishedVersion | en_US |
cristin.ispublished | true | |
cristin.fulltext | original | |
cristin.qualitycode | 1 | |
dc.identifier.doi | 10.3390/universe8090440 | |
dc.identifier.cristin | 2059860 | |
dc.source.journal | Universe | en_US |
dc.source.volume | 8 | en_US |
dc.source.issue | 9 | en_US |
dc.source.pagenumber | 25 | en_US |