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Shell-model structure of exotic nuclei beyond 132Sn

2007/11/01 by A. Covello, L. Coraggio, A. Gargano +1 · 6 citations
Physics and Astronomy · #Atomic and Molecular Physics #Atomic physics #Excited state #MAGIC (telescope) #Materials science #Nuclear physics #Nuclear physics research studies #Nuclear shell model #Nuclear structure #Nucleon #Particle physics #Physics #Quantum Chromodynamics and Particle Interactions #Quantum mechanics #Range (aeronautics) #SHELL model #Statistical physics #nucl-th

paper · pdf · doi:10.1140/epjst/e2007-00275-7

published in The European Physical Journal Special Topics 150(1), 93-96 (Springer Science+Business Media) · 4 pages, 1 figure, 2 tables, talk given at 7th International Conference on Radioactive Nuclear Beams, Cortina d'Ampezzo (Italy), July 3-7 2006

openalex publication_date 2007/11/01 · arxiv created 2008/01/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We report on a study of exotic nuclei around doubly magic 132Sn in terms of the shell model employing a realistic effective interaction derived from the CD-Bonn nucleon-nucleon potential. The short-range repulsion of the bare potential is renormalized by constructing a smooth low-momentum potential, V-low-k, that is used directly as input for the calculation of the effective interaction. In this paper we focus attention on the nuclei 134Sn and 135Sb which, with an N/Z ratio of 1.68 and 1.65, respectively, are at present the most exotic nuclei beyond 132Sn for which information exists on excited states. Comparison shows that the calculated results for both nuclei are in very good agreement with the experimental data. We present our predictions of the hitherto unknown spectrum of 136Sn.

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