Neutral-current supernova neutrino-nucleus scattering off 127I and 133Cs
| dc.contributor.author | Hellgren, Matti | |
| dc.contributor.author | Suhonen, Jouni | |
| dc.date.accessioned | 2022-10-24T10:37:09Z | |
| dc.date.available | 2022-10-24T10:37:09Z | |
| dc.date.issued | 2022 | |
| dc.identifier.citation | Hellgren, 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.other | CONVID_159269716 | |
| dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/83639 | |
| dc.description.abstract | A 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.mimetype | application/pdf | |
| dc.language.iso | eng | |
| dc.publisher | American Physical Society (APS) | |
| dc.relation.ispartofseries | Physical Review C | |
| dc.rights | In Copyright | |
| dc.title | Neutral-current supernova neutrino-nucleus scattering off 127I and 133Cs | |
| dc.type | research article | |
| dc.identifier.urn | URN:NBN:fi:jyu-202210244950 | |
| 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 | 2469-9985 | |
| dc.relation.numberinseries | 2 | |
| dc.relation.volume | 106 | |
| dc.type.version | publishedVersion | |
| dc.rights.copyright | ©2022 American Physical Society | |
| dc.rights.accesslevel | openAccess | fi |
| dc.type.publication | article | |
| dc.relation.grantnumber | 318043 | |
| dc.subject.yso | astrofysiikka | |
| dc.subject.yso | ydinfysiikka | |
| dc.subject.yso | neutriinot | |
| dc.subject.yso | sironta | |
| dc.subject.yso | supernovat | |
| dc.subject.yso | hiukkasfysiikka | |
| dc.format.content | fulltext | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p20188 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p5219 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p1026 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p10347 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
| dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
| dc.relation.doi | 10.1103/PhysRevC.106.025808 | |
| dc.relation.funder | Research Council of Finland | en |
| dc.relation.funder | Suomen Akatemia | fi |
| jyx.fundingprogram | Academy Project, AoF | en |
| jyx.fundingprogram | Akatemiahanke, SA | fi |
| jyx.fundinginformation | This 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.okm | A1 |
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