Spectrum-shape method and the next-to-leading-order terms of the β-decay shape factor
Abstract
Effective values of the axial-vector coupling constant gA have lately attracted much attention due to the prominent role of gA in determining the half-lives of double β decays, in particular their neutrinoless mode. The half-life method, i.e., comparing the calculated half-lives to the corresponding experimental ones, is the most widely used method to access the effective values of gA. The present paper investigates the possibilities offered by a complementary method: the spectrum-shape method (SSM). In the SSM, comparison of the shapes of the calculated and measured β electron spectra of forbidden nonunique β decays yields information on the magnitude of gA. In parallel, we investigate the impact of the next-to-leading-order terms of the β-decay shape function and the radiative corrections on the half-life method and the SSM by analyzing the fourfold forbidden decays of 113Cd and 115In by using three nuclear-structure theory frameworks; namely, the nuclear shell model, the microscopic interacting boson-fermion model, and the microscopic quasiparticle-phonon model. The three models yield a consistent result, gA≈0.92, when the SSM is applied to the decay of 113Cd for which β-spectrum data are available. At the same time the half-life method yields results which are in tension with each other and the SSM result.
Main Authors
Format
Articles
Research article
Published
2017
Series
Subjects
Publication in research information system
Publisher
American Physical Society
The permanent address of the publication
https://urn.fi/URN:NBN:fi:jyu-201703071595Käytä tätä linkitykseen.
Review status
Peer reviewed
ISSN
2469-9985
DOI
https://doi.org/10.1103/PhysRevC.95.024327
Language
English
Published in
Physical Review C
Citation
- Haaranen, M., Kotila, J.-M., & Suhonen, J. (2017). Spectrum-shape method and the next-to-leading-order terms of the β-decay shape factor. Physical Review C, 95(2), Article 024327. https://doi.org/10.1103/PhysRevC.95.024327
Copyright© 2017 American Physical Society. Published in this repository with the kind permission of the publisher.