dc.contributor.author | Enckell, Vera-Maria | |
dc.contributor.author | Nurmi, Sami | |
dc.contributor.author | Räsänen, Syksy | |
dc.contributor.author | Tomberg, Eemeli | |
dc.date.accessioned | 2021-04-16T10:56:42Z | |
dc.date.available | 2021-04-16T10:56:42Z | |
dc.date.issued | 2021 | |
dc.identifier.citation | Enckell, V.-M., Nurmi, S., Räsänen, S., & Tomberg, E. (2021). Critical point Higgs inflation in the Palatini formulation. <i>Journal of High Energy Physics</i>, <i>2021</i>(4), Article 59. <a href="https://doi.org/10.1007/jhep04(2021)059" target="_blank">https://doi.org/10.1007/jhep04(2021)059</a> | |
dc.identifier.other | CONVID_66432764 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/75089 | |
dc.description.abstract | We study Higgs inflation in the Palatini formulation with the renormalisation group improved potential in the case when loop corrections generate a feature similar to an inflection point. Assuming that there is a threshold correction for the Higgs quartic coupling λ and the top Yukawa coupling yt, we scan the three-dimensional parameter space formed by the two jumps and the non-minimal coupling ξ.
The spectral index ns can take any value in the observationally allowed range. The lower limit for the running is αs > −3.5 × 10−3, and αs can be as large as the observational upper limit. Running of the running is small. The tensor-to-scalar ratio is 2.2×10−17 < r < 2 × 10−5. We find that slow-roll can be violated near the feature, and a possible period of ultra-slow-roll contributes to the widening of the range of CMB predictions. Nevertheless, for the simplest tree-level action, the Palatini formulation remains distinguishable from the metric formulation even when quantum corrections are taken into account, because of the small tensor-to-scalar ratio. | en |
dc.format.mimetype | application/pdf | |
dc.language | eng | |
dc.language.iso | eng | |
dc.publisher | Springer | |
dc.relation.ispartofseries | Journal of High Energy Physics | |
dc.rights | CC BY 4.0 | |
dc.subject.other | cosmology of theories beyond the SM | |
dc.subject.other | renormalization group | |
dc.title | Critical point Higgs inflation in the Palatini formulation | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-202104162394 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 1126-6708 | |
dc.relation.numberinseries | 4 | |
dc.relation.volume | 2021 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © The Authors. Article funded by SCOAP3 | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.subject.yso | teoreettinen fysiikka | |
dc.subject.yso | kosmologia | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p38202 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p7160 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1007/jhep04(2021)059 | |
dc.type.okm | A1 | |