| Issue |
EPJ Web Conf.
Volume 342, 2025
14th International Spring Seminar on Nuclear Physics “Cutting-Edge Developments in Nuclear Structure Physics”
|
|
|---|---|---|
| Article Number | 01026 | |
| Number of page(s) | 8 | |
| DOI | https://doi.org/10.1051/epjconf/202534201026 | |
| Published online | 21 November 2025 | |
https://doi.org/10.1051/epjconf/202534201026
Nuclear structure investigations in the A ≈ 30 mass region
1 Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences, BG-1784, Sofia, Bulgaria
2 INFN, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Italy
3 Dipartimento di Matematica e Fisica, Università degli Studi della Campania “Luigi Vanvitelli”, I-8110 Caserta, Italy
4 INFN, Sezione di Napoli, I-80126 Napoli, Italy
5 CSNSM, CNRS/Université, Paris-Sud XI, 91405 Orsay Campus, France
* Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Published online: 21 November 2025
Abstract
Experimental results for the structure of nuclei in the mass region A ≈ 30 are presented. The first part of the paper is dedicated to the mirror nuclei 31S and 31P. In the second part we focus on the structure of the N=Z nucleus of 30P. Excited states in the 30P, 31P and 31S were populated in the same experiment as the 1pn, 1p and 1n exit channels of the reaction 20Ne + 12C, respectively. The 20Ne beam accelerated to an energy of 33 MeV was delivered by the Piave-Alpi accelerator of the Laboratori Nazionali di Legnaro. Results for branching ratios measurements, angular correlations analysis of coincident γ-rays as well as Doppler-shift attenuation lifetime measurements are reported. The γ-rays were detected using the multi-detector array GASP with the EUCLIDES charged particle detector. The isospin symmetry in A=31 mirror nuclei was investigated using the Equation of Motion method based on a chiral potential and including two- and three-body forces. The level scheme and branching ratios for the positive parity band in the N=Z nucleus of 30P are well reproduced by the shell model calculations.
© The Authors, published by EDP Sciences, 2025
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