dc.contributor.author | Kostensalo, Joel | |
dc.contributor.author | Suhonen, Jouni | |
dc.contributor.author | Volkmer, Juliane | |
dc.contributor.author | Zatschler, Stefan | |
dc.contributor.author | Zuber, Kai | |
dc.date.accessioned | 2021-09-28T11:51:41Z | |
dc.date.available | 2021-09-28T11:51:41Z | |
dc.date.issued | 2021 | |
dc.identifier.citation | Kostensalo, J., Suhonen, J., Volkmer, J., Zatschler, S., & Zuber, K. (2021). Confirmation of gA quenching using the revised spectrum-shape method for the analysis of the 113Cd β-decay as measured with the COBRA demonstrator. <i>Physics Letters B</i>, <i>822</i>, Article 136652. <a href="https://doi.org/10.1016/j.physletb.2021.136652" target="_blank">https://doi.org/10.1016/j.physletb.2021.136652</a> | |
dc.identifier.other | CONVID_101214144 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/77944 | |
dc.description.abstract | In this article we present an updated spectrum-shape analysis of the113Cd fourfold forbidden non-uniqueβ-decay transition in order to address the quenching of the weak axial-vector coupling gA in low-momentum exchange nuclear processes. The experimental data were collected in a dedicated low-threshold run with the COBRA demonstrator at the LNGS and resulted in 44 individual113Cdspectra. These data are evaluated in the context of three nuclear model frameworks based on a revised version of the spectrum-shape method and the conserved vector current hypothesis. The novel idea devised in the present work is to fit the value of the small relativistic nuclear matrix element (s-NME) driving the nuclear model calculations, which remained essentially as a free parameter in previous studies. This is done by tuning the nuclear structure calculations and making use of the interplay of gA and the s-NME such that the experimentally known113Cd half-life gets reproducible by the different frameworks. In this way, a best fit s-NME value can be derived for each of the considered nuclear models, which finally enters the template calculations used to perform the spectrum-shape analysis for each of the obtained113Cd spectra. The primary analysis strategy results in significantly quenched values of the axial-vector coupling for all three nuclear models: gA(ISM)=0.907±0.064,gA(MQPM)=0.993±0.063andgA(IBFM-2)=0.828±0.140. Moreover, with our data-driven approach one of the main shortcomings of the spectrum-shape method has been resolved. This achievement is a milestone in the description of strongly forbiddenβ-decays and adds to the indications for the existence of a quenching of gA in low-momentum exchange nuclear processes. | en |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Elsevier | |
dc.relation.ispartofseries | Physics Letters B | |
dc.rights | CC BY 4.0 | |
dc.subject.other | 113Cd β-decay | |
dc.subject.other | axial-vector coupling | |
dc.subject.other | gA quenching | |
dc.subject.other | spectrum-shape method | |
dc.subject.other | CdZnTe | |
dc.subject.other | COBRA | |
dc.title | Confirmation of gA quenching using the revised spectrum-shape method for the analysis of the 113Cd β-decay as measured with the COBRA demonstrator | |
dc.type | article | |
dc.identifier.urn | URN:NBN:fi:jyu-202109285011 | |
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 | 0370-2693 | |
dc.relation.volume | 822 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2021 The Authors. Published by Elsevier B.V. | |
dc.rights.accesslevel | openAccess | fi |
dc.relation.grantnumber | 318043 | |
dc.subject.yso | ydinfysiikka | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1016/j.physletb.2021.136652 | |
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 | the collaboration would like tothank the German Research Foundation (Deutsche Forschungs-gemeinschaft, DFG) for its past funding and the support of theCOBRA XDEM upgrade under the project numbers ZU123/3and GO1133/1. Additionally, the support by the Academy of Finland under the project number 318043 and from the Jennyand Antti Wihuri Foundation is acknowledged. | |
dc.type.okm | A1 | |