113Cdβ-decay spectrum and gA quenching using spectral moments

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.
Main Authors
Format
Articles Research article
Published
2023
Series
Subjects
Publication in research information system
Publisher
American Physical Society (APS)
The permanent address of the publication
https://urn.fi/URN:NBN:fi:jyu-202306224087Käytä tätä linkitykseen.
Review status
Peer reviewed
ISSN
2469-9985
DOI
https://doi.org/10.1103/PhysRevC.107.055502
Language
English
Published in
Physical Review C
Citation
License
In CopyrightOpen Access
Additional information about funding
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.
Copyright© 2023 American Physical Society (APS)

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