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DOE OSTI · 2339932

Ne 21 energy levels approaching the α -particle threshold

Abstract

Nuclei around Ne 20 exhibit an interplay of different excitations caused by different aspects of nuclear structure, including single-particle and multiparticle configurations and collective rotations. One-nucleon transfer reactions selectively probe single-particle structures in these nuclei. These nuclei are also important to astrophysics, with a number of important reactions proceeding through this mass region. Energy levels approaching the α -particle threshold in Ne 21 are of importance to nuclear structure. The Ne 20 ( d , p ) Ne 21 reaction was measured and the corresponding spectroscopic nuclear information was extracted. States in Ne 21 were populated using the Ne 20 ( d , p ) Ne 21 reaction in forward kinematics. Protons were identified in the Triangle Universities Nuclear Laboratory (TUNL) Enge split-pole spectrograph and angular distributions were extracted. Spin-party assignments were made and neutron partial widths were determined based on distorted-wave Born approximation (DWBA) analysis. Several new energy levels were observed at energies of 7176, 7235, 7250, and 7337 keV, and spin-parities are reported which generally agree with previous results where literature was available. Spin and parity assignments are reported for several energy levels along with estimated neutron widths for those states above the neutron threshold ( S n = 6761 keV ). Results from this study are placed in context with a review of the available literature on all known states in this energy region of Ne 21 . Published by the American Physical Society 2024

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BibTeXRIS

Angus, C. (ORCID:0000000307784429), Frost-Schenk, J., Laird, A. M. (ORCID:000000030423363X), Adsley, P. (ORCID:000000031373679X), Longland, R. (ORCID:000000017731580X), Barton, C. J., Diget, C. Aa., Marshall, C., Portillo Chaves, F. (ORCID:0000000235687952), Setoodehnia, K. (ORCID:0000000221495060). 2024-04-22. Ne 21 energy levels approaching the α -particle threshold. https://doi.org/10.1103/physrevc.109.044323

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