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Cross-shell excited states in 32Si and 29Al populated using fusion-evaporation
TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada..
KTH, School of Engineering Sciences (SCI), Physics, Nuclear Science and Engineering. Indian Inst Technol Roorkee, Dept Phys, Roorkee 247667, India..ORCID iD: 0000-0002-4590-5917
Simon Fraser Univ, Dept Chem, 8888 Univ Dr, Burnaby, BC V5A 1S6, Canada..
2025 (English)In: Nuclear Physics A, ISSN 0375-9474, E-ISSN 1873-1554, Vol. 1057, article id 123042Article in journal (Refereed) Published
Abstract [en]

In the neutron-rich sd shell near the N = 20 'island of inversion', the evolution of the N = 20 shell gap is indicated by the energies of negative-parity states which primarily arise due to single neutron excitation to higher lying orbitals across the shell gap. These negative-parity states often have high spin (due to the participation of the 0f7/2 orbital) and are therefore preferentially populated using fusion-evaporation reactions. We have studied the intermediate energy levels of 32Si and 29Al using 12C(22Ne,2p) and 12C(22Ne,alpha p) reactions, identifying several negative-parity states in both nuclides.

Place, publisher, year, edition, pages
Elsevier BV , 2025. Vol. 1057, article id 123042
Keywords [en]
Fusion-evaporation, Gamma-ray spectroscopy, Cross-shell excitation, Shell evolution
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-361045DOI: 10.1016/j.nuclphysa.2025.123042ISI: 001428714800001Scopus ID: 2-s2.0-85217791260OAI: oai:DiVA.org:kth-361045DiVA, id: diva2:1943604
Note

QC 20250311

Available from: 2025-03-11 Created: 2025-03-11 Last updated: 2025-03-11Bibliographically approved

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Choudhary, Priyanka

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