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dc.contributor.authorCUPID-Mo Collaboration
dc.date.accessioned2023-10-26T05:11:49Z
dc.date.available2023-10-26T05:11:49Z
dc.date.issued2023
dc.identifier.citationCUPID-Mo Collaboration. (2023). Measurement of the 2νββ Decay Rate and Spectral Shape of 100Mo from the CUPID-Mo Experiment. <i>Physical Review Letters</i>, <i>131</i>, Article 162501. <a href="https://doi.org/10.1103/PhysRevLett.131.162501" target="_blank">https://doi.org/10.1103/PhysRevLett.131.162501</a>
dc.identifier.otherCONVID_194173453
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/90667
dc.description.abstractNeutrinoless double beta decay (0νββ) is a yet unobserved nuclear process that would demonstrate Lepton number violation, a clear evidence of beyond standard model physics. The process two neutrino double beta decay (2νββ) is allowed by the standard model and has been measured in numerous experiments. In this Letter, we report a measurement of 2νββ decay half-life of 100Mo to the ground state of 100Ru of [7.07±0.02(stat)±0.11(syst)]×1018  yr by the CUPID-Mo experiment. With a relative precision of ±1.6% this is the most precise measurement to date of a 2νββ decay rate in 100Mo. In addition, we constrain higher-order corrections to the spectral shape, which provides complementary nuclear structure information. We report a novel measurement of the shape factor ξ3,1=0.45±0.03(stat)±0.05(syst) based on a constraint on the ratio of higher-order terms from theory, which can be reliably calculated. This is compared to theoretical predictions for different nuclear models. We also extract the first value for the effective axial vector coupling constant obtained from a spectral shape study of 2νββ decay.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review Letters
dc.rightsIn Copyright
dc.titleMeasurement of the 2νββ Decay Rate and Spectral Shape of 100Mo from the CUPID-Mo Experiment
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202310266696
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosKoulutuksen tutkimuslaitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.laitosFinnish Institute for Educational Researchen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0031-9007
dc.relation.volume131
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber314733
dc.relation.grantnumber320062
dc.relation.grantnumber345869
dc.subject.ysoydinfysiikka
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevLett.131.162501
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundinginformationThis work has been performed in the framework of the CUPID-1 and P2IO LabEx programs, funded by the Agence Nationale de la Recherche (ANR, France). F. A. D., V. V. K., V. I. T., and M. M. Z. were supported in part by the National Research Foundation of Ukraine. A. S. B., S. I. K., I. M. M., V. N. S., and V. I. U. were supported by the Russian Science Foundation. J. K. is supported by Academy of Finland. F. D. was partly supported by the Slovak Research and Development Agency. Additionally the work is supported by the Istituto Nazionale di Fisica Nucleare (INFN), by the US Department of Energy (DOE) Office of Science. This work makes use of the Diana data analysis software and the background model based on JAGS, developed by the CUORICINO, CUORE, LUCIFER, and CUPID-0 collaborations.
dc.type.okmA1


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