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dc.contributor.authorCOBRA collaboration
dc.date.accessioned2020-01-02T11:55:08Z
dc.date.available2020-01-02T11:55:08Z
dc.date.issued2020
dc.identifier.citationCOBRA collaboration. (2020). Quenching of gA deduced from the β-spectrum shape of 113Cd measured with the COBRA experiment. <i>Physics Letters B</i>, <i>800</i>, Article 135092. <a href="https://doi.org/10.1016/j.physletb.2019.135092" target="_blank">https://doi.org/10.1016/j.physletb.2019.135092</a>
dc.identifier.otherCONVID_33934754
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/67073
dc.description.abstractA dedicated study of the quenching of the weak axial-vector coupling strength gA in nuclear processes has been performed by the COBRA collaboration. This investigation is driven by nuclear model calculations which show that the β-spectrum shape of the fourfold forbidden non-unique decay of 113Cd strongly depends on the effective value of gA. Using an array of CdZnTe semiconductor detectors, 45 independent 113Cd spectra were obtained and interpreted in the context of three nuclear models. The resulting effective mean values are g‾A(ISM)=0.915±0.007, g‾A(MQPM)=0.911±0.013 and g‾A(IBFM-2)=0.955±0.022. These values agree well within the determined uncertainties and deviate significantly from the free value of gA. This can be seen as a first step towards answering the long-standing question regarding quenching effects related to gA in low-energy nuclear processes.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.subject.other113Cd beta-decay
dc.subject.otheraxial-vector coupling
dc.subject.othergA quenching
dc.subject.otherspectrum-shape method
dc.subject.otherCdZnTe
dc.subject.otherCOBRA
dc.titleQuenching of gA deduced from the β-spectrum shape of 113Cd measured with the COBRA experiment
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202001021007
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.issn0370-2693
dc.relation.volume800
dc.type.versionpublishedVersion
dc.rights.copyright© 2019 The Author
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber318043
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.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2019.135092
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationCOBRA is supported by the German Research Foundation DFG (ZU123/3 and GO1133/1) and by the Ministry of Education, Youth and Sports of the Czech Republic with contract no. CZ.02.1.01/0.0/0.0/16_013/0001733. Additionally, support from the Academy of Finland under the project no. 318043 and from the Jenny and Antti Wihuri Foundation is acknowledged.
dc.type.okmA1


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