Low-spin excitations in 89Br populated in β−decay of 89Se
Rząca-Urban, T., Sieja, K., Czerwiński, M., Kurpeta, J., Pomorski, M., Urban, W., Wiśniewski, J., Wróblewski, M., Canete, L., Eronen, T., Geldhof, S., Jokinen, A., Kankainen, A., Moore, I. D., Nesterenko, D., Penttilä, H., Pohjalainen, I., Rinta-Antila, S., de Roubin, A., & Vilén, M. (2022). Low-spin excitations in 89Br populated in β−decay of 89Se. Physical Review C, 106(2), Article 024322. https://doi.org/10.1103/PhysRevC.106.024322
Julkaistu sarjassa
Physical Review CTekijät
Päivämäärä
2022Tekijänoikeudet
©2022 American Physical Society
Low-spin, excited states of the 89Br nucleus, populated in β− decay of 89Se have been studied for the first time. The 89Se nuclei were produced in proton-induced fission of natural thorium using the IGISOL facility and separated using a dipole magnet and the coupled JYFLTRAP Penning trap. Gamma radiation following the β− decay of 89Se was measured with an array of high-resolution germanium detectors. Levels scheme of 89Br was extended by 12 new levels and 31 new γ transitions. Spin-parity (3/2+) has been proposed for the ground state of the 89Se mother nucleus, replacing the (5/2+) assignment reported in data bases. The observed Gamow-Teller β− transition to the 1754.5-keV level indicates a πg9/2-based configuration. The level scheme of 89Br has been compared to large scale shell-model calculations. Excitations based on πp3/2 and πf5/2 single-particle levels as well as their anomalous coupling are proposed to explain the low-energy excitation scheme of 89Br.
Julkaisija
American Physical Society (APS)ISSN Hae Julkaisufoorumista
2469-9985Asiasanat
Julkaisu tutkimustietojärjestelmässä
https://converis.jyu.fi/converis/portal/detail/Publication/151755186
Metadata
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Rahoittaja(t)
Suomen Akatemia; Euroopan komissioRahoitusohjelmat(t)
Akatemiatutkijan tutkimuskulut, SA; Akatemiatutkija, SA
The content of the publication reflects only the author’s view. The funder is not responsible for any use that may be made of the information it contains.
Lisätietoja rahoituksesta
This work has been supported by the National Science Centre under Contract No. DEC-2018/29/N/ST2/00707 and by the Academy of Finland under the Finnish Centre of Excellence Program 2012–2017 (Nuclear and Accelerator Based Physics Research at JYFL) and under Grants No. 275389, No. 284516, No. 312544, and No. 295207. This project has received funding from the European Union's Horizon 2020 European Nuclear Science and Application Research 2 under Grant Agreement No. 654002 (ENSAR2). ...Lisenssi
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