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dc.contributor.authorHellgren, Matti
dc.contributor.authorSuhonen, Jouni
dc.date.accessioned2022-10-24T10:37:09Z
dc.date.available2022-10-24T10:37:09Z
dc.date.issued2022
dc.identifier.citationHellgren, M., & Suhonen, J. (2022). Neutral-current supernova neutrino-nucleus scattering off 127I and 133Cs. <i>Physical Review C</i>, <i>106</i>(2), Article 025808. <a href="https://doi.org/10.1103/PhysRevC.106.025808" target="_blank">https://doi.org/10.1103/PhysRevC.106.025808</a>
dc.identifier.otherCONVID_159269716
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/83639
dc.description.abstractA large number of the presently running neutrino and dark-matter experiments use thallium-doped cesium-iodide CsI[Tl] crystals, sodium-doped cesium-iodide CsI[Na] crystals, or thallium-doped sodium-iodide NaI[Tl] crystals. In the present paper we calculate elastic and inelastic cross sections for neutral-current supernova-neutrino scattering off 127I and 133Cs, relevant for experiments using CsI[Tl], CsI[Na], or NaI[Tl] crystals. We study also the cross sections folded with two-parameter Fermi-Dirac distributions of the supernova-neutrino spectrum. The adopted nuclear-theory framework is the microscopic quasiparticle-phonon model, able to operate in large single-particle valence bases and use G-matrix based two-nucleon interactions with a phenomenological renormalization.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.titleNeutral-current supernova neutrino-nucleus scattering off 127I and 133Cs
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202210244950
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries2
dc.relation.volume106
dc.type.versionpublishedVersion
dc.rights.copyright©2022 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber318043
dc.subject.ysoastrofysiikka
dc.subject.ysoydinfysiikka
dc.subject.ysoneutriinot
dc.subject.ysosironta
dc.subject.ysosupernovat
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p20188
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p5219
jyx.subject.urihttp://www.yso.fi/onto/yso/p1026
jyx.subject.urihttp://www.yso.fi/onto/yso/p10347
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.106.025808
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationThis work has been partially supported by the Academy of Finland under Project No. 318043. M.H. acknowledges financial support from the Väisälä Foundation.
dc.type.okmA1


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