Abstract:The level structure of the neutron-rich 77 Cu nucleus is investigated through β-delayed γ-ray spectroscopy at the Radioactive Isotope Beam Factory of the RIKEN Nishina Center. Ions of 77 Ni are produced by inflight fission, separated and identified in the BigRIPS fragment separator, and implanted in the WAS3ABi silicon detector array, surrounded by Ge cluster detectors of the EURICA array. A large number of excited states in 77 Cu are identified for the first time by correlating γ rays with the β decay of 77 N… Show more
“…In nuclear medium, the isovector correction based on the meson-exchange picture is made usually: g ℓ (p) = g free ℓ (p) + δg ℓ and g ℓ (n) = g free ℓ (n) − δg ℓ [35,36], with the empirical value of δg ℓ being between 0 [38] and 0.1 [37]. The measured magnetic moments of 75 Cu are 1.40 (6)µ N for the first 3/2 − state as obtained by the present work, and 1.0062 (13)µ N for the first 5/2 − state [11]. We can evaluate the values of q s and δg ℓ from them.…”
“…In nuclear medium, the isovector correction based on the meson-exchange picture is made usually: g ℓ (p) = g free ℓ (p) + δg ℓ and g ℓ (n) = g free ℓ (n) − δg ℓ [35,36], with the empirical value of δg ℓ being between 0 [38] and 0.1 [37]. The measured magnetic moments of 75 Cu are 1.40 (6)µ N for the first 3/2 − state as obtained by the present work, and 1.0062 (13)µ N for the first 5/2 − state [11]. We can evaluate the values of q s and δg ℓ from them.…”
“…After the first production of 78 Ni 17 , enormous efforts have been put into investigating its structure. Previous measurements indirectly inferred persistent N = 50 [18][19][20][21][22] and Z = 28 [23][24][25] shell closures at 78 Ni. This notion has been reinforced theoretically by ab initio predictions 27 .…”
Characterisation of the few doubly magic nuclei, known and predicted, provides a benchmark for our knowledge of the fundamental forces that drive the evolution of shell closures with proton-to-neutron asymme
“…The Z = 28 shell closure is well known for exhibiting a strong magic behavior. However, in Cu isotopes (Z = 29), the lowering of the 1 f 5/2 orbital induces a reduction of ≈2 MeV of the Z = 28 shell gap between N = 40 and N = 50 [12]. Further, many efforts have been devoted to the characterization of the N = 50 shell gap [13][14][15][16][17][18][19][20] and support a possible weakening of the gap at Z = 32 [21,22], whereas a persistent N = 50 gap has been suggested at Z = 30 [19].…”
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