Two-neutrino ββ decay of 136Xe to the first excited 0+ state in 136Ba
Abstract
We calculate the nuclear matrix element for the two-neutrino ββ decay of 136Xe into the first excited 0+ state of 136Ba. We use different many-body methods: the quasiparticle random-phase approximation (QRPA) framework, the nuclear shell model, the interacting boson model (IBM-2), and an effective field theory (EFT) for β and ββ decays. While the QRPA suggests a decay rate at the edge of current experimental limits, the shell model points to a half-life about two orders of magnitude longer. The predictions of the IBM-2 and the EFT lie in between, and the latter provides systematic uncertainties at leading order. An analysis of the running sum of the nuclear matrix element indicates that subtle cancellations between the contributions of intermediate states can explain the different theoretical predictions. For the EFT, we also present results for two-neutrino ββ decays to the first excited 0+ state in other nuclei.
Main Authors
Format
Articles
Research article
Published
2023
Series
Subjects
Publication in research information system
Publisher
Elsevier
The permanent address of the publication
https://urn.fi/URN:NBN:fi:jyu-202301191392Käytä tätä linkitykseen.
Review status
Peer reviewed
ISSN
0370-2693
DOI
https://doi.org/10.1016/j.physletb.2023.137689
Language
English
Published in
Physics Letters B
Citation
- Jokiniemi, L., Romeo, B., Brase, C., Kotila, J., Soriano, P., Schwenk, A., & Menéndez, J. (2023). Two-neutrino ββ decay of 136Xe to the first excited 0+ state in 136Ba. Physics Letters B, 838, Article 137689. https://doi.org/10.1016/j.physletb.2023.137689
Funder(s)
Research Council of Finland
Research Council of Finland
Funding program(s)
Research costs of Academy Research Fellow, AoF
Academy Research Fellow, AoF
Akatemiatutkijan tutkimuskulut, SA
Akatemiatutkija, SA
![Research Council of Finland Research Council of Finland](/jyx/themes/jyx/images/funders/sa_logo.jpg?_=1739278984)
Additional information about funding
This work was supported by the Arthur B. McDonald Canadian Astroparticle Physics Research Institute, the Academy of Finland (Grant Nos. 314733 and 345869), by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (Grant Agreement No. 101020842 and No. 951281), by the “Ramón y Cajal” program with grant RYC-2017-22781, and grants CEX2019-000918-M, PID2020-118758GB-I00 and and RTI2018-095979-B-C41 funded by MCIN/AEI/10.13039/501100011033 and by “ESF Investing in your future”. TRIUMF receives funding via a contribution through the National Research Council of Canada.
Copyright© 2023 The Author(s). Published by Elsevier B.V.