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dc.contributor.authorKostensalo, Joel
dc.contributor.authorLisi, Eligio
dc.contributor.authorMarrone, Antonio
dc.contributor.authorSuhonen, Jouni
dc.date.accessioned2023-06-22T09:00:59Z
dc.date.available2023-06-22T09:00:59Z
dc.date.issued2023
dc.identifier.citationKostensalo, J., Lisi, E., Marrone, A., & Suhonen, J. (2023). 113Cdβ-decay spectrum and gA quenching using spectral moments. <i>Physical Review C</i>, <i>107</i>(5), Article 055502. <a href="https://doi.org/10.1103/PhysRevC.107.055502" target="_blank">https://doi.org/10.1103/PhysRevC.107.055502</a>
dc.identifier.otherCONVID_183664878
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/88032
dc.description.abstractWe present an alternative analysis of the 113Cdβ-decay electron energy spectrum in terms of spectral moments μn, corresponding to the averaged values of nth powers of the β particle energy. The zeroth moment μ0 is related to the decay rate, while higher moments μn are related to the spectrum shape. The here advocated spectral-moment method (SMM) allows for a complementary understanding of previous results, obtained using the so-called spectrum-shape method (SSM) and its revised version, in terms of two free parameters: r=gA/gV (the ratio of axial-vector to vector couplings) and s (the small vectorlike relativistic nuclear matrix element, s-NME). We present numerical results for three different nuclear models with the conserved vector current hypothesis (CVC) assumption of gV=1. We show that most of the spectral information can be captured by the first few moments, which are simple quadratic forms (conic sections) in the (r,s) plane: An ellipse for n=0 and hyperbolas for n≥1, all being nearly degenerate as a result of cancellations among nuclear matrix elements. The intersections of these curves, as obtained by equating theoretical and experimental values of μn, identify the favored values of (r,s) at a glance, without performing detailed fits. In particular, we find that values around r≈1 and s≈1.6 are consistently favored in each nuclear model, confirming the evidence for gA quenching in 113Cd, and shedding light on the role of the s-NME. We briefly discuss future applications of the SMM to other forbidden β-decay spectra sensitive to gA.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.title113Cdβ-decay spectrum and gA quenching using spectral moments
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202306224087
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.numberinseries5
dc.relation.volume107
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 American Physical Society (APS)
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.107.055502
jyx.fundinginformationThe work of E.L. and A.M. is partly supported the Italian Ministero dell’Università e Ricerca (MUR) through the research Grant No. 2017W4HA7S, “NAT-NET: Neu trino and Astroparticle Theory Network” under the program PRIN 2017, and by the Istituto Nazionale di Fisica Nucle are (INFN) through the “Theoretical Astroparticle Physics” (TAsP) project.
dc.type.okmA1


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