113Cdβ-decay spectrum and gA quenching using spectral moments
dc.contributor.author | Kostensalo, Joel | |
dc.contributor.author | Lisi, Eligio | |
dc.contributor.author | Marrone, Antonio | |
dc.contributor.author | Suhonen, Jouni | |
dc.date.accessioned | 2023-06-22T09:00:59Z | |
dc.date.available | 2023-06-22T09:00:59Z | |
dc.date.issued | 2023 | |
dc.identifier.citation | Kostensalo, 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.other | CONVID_183664878 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/88032 | |
dc.description.abstract | We 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.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 | 113Cdβ-decay spectrum and gA quenching using spectral moments | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-202306224087 | |
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 | 5 | |
dc.relation.volume | 107 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2023 American Physical Society (APS) | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.subject.yso | ydinfysiikka | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
dc.relation.doi | 10.1103/PhysRevC.107.055502 | |
jyx.fundinginformation | The 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.okm | A1 |