Consequences of the improved limits on the tnsor-to-scalar ratio from BICEP/Planck, and of future CMB-S4 measurements, for inflationary models

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

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