TY - JOUR
T1 - Position of the single-particle 3/2− state in 135Sn and the N=90 subshell closure
AU - Jungclaus, A.
AU - Doornenbal, P.
AU - Acosta, J.
AU - Vaquero, V.
AU - Browne, F.
AU - Cortes, M.L.
AU - Gargano, A.
AU - Koiwai, T.
AU - Naïdja, H.
AU - Taniuchi, R.
AU - Tostevin, J.A.
AU - Wimmer, K.
AU - Algora, A.
AU - Baba, H.
AU - Fernández, A.
AU - Lalovic, N.
AU - Nacher, E.
AU - Rubio, B.
AU - Sakurai, H.
N1 - © 2024 The Author(s).
PY - 2024/4/1
Y1 - 2024/4/1
N2 - The decay of excited states of the nucleus 135Sn, with three neutrons outside the doubly-magic 132Sn core, was studied in an experiment performed at the Radioactive Isotope Beam Factory at RIKEN. Several γ rays emitted from excited 135Sn ions were observed following one-neutron and one-neutron-one-proton removal from 136Sn and 137Sb beams, respectively, on a beryllium target at relativistic energies. Based on the analogy to 133Sn populated via one-neutron removal from 134Sn, an excitation energy of 695(15) keV is assigned to the 3/2− state with strongest single-particle character in 135Sn. This result provides the first direct information about the evolution of the neutron shell structure beyond N=82 and thus allows for a crucial test of shell-model calculations in this region. The experimental findings are in full agreement with calculations performed employing microscopic effective two-body interactions derived from CD-Bonn and N3LO nucleon-nucleon potentials, which do not predict a pronounced subshell gap at neutron number N=90. The occurrence of such a gap in 140Sn, i.e., when the 1f7/2 orbital is completely filled, had been proposed in the past, in analogy to the magicity of 48Ca, featuring a completely filled 0f7/2 orbital one harmonic oscillator shell below.
AB - The decay of excited states of the nucleus 135Sn, with three neutrons outside the doubly-magic 132Sn core, was studied in an experiment performed at the Radioactive Isotope Beam Factory at RIKEN. Several γ rays emitted from excited 135Sn ions were observed following one-neutron and one-neutron-one-proton removal from 136Sn and 137Sb beams, respectively, on a beryllium target at relativistic energies. Based on the analogy to 133Sn populated via one-neutron removal from 134Sn, an excitation energy of 695(15) keV is assigned to the 3/2− state with strongest single-particle character in 135Sn. This result provides the first direct information about the evolution of the neutron shell structure beyond N=82 and thus allows for a crucial test of shell-model calculations in this region. The experimental findings are in full agreement with calculations performed employing microscopic effective two-body interactions derived from CD-Bonn and N3LO nucleon-nucleon potentials, which do not predict a pronounced subshell gap at neutron number N=90. The occurrence of such a gap in 140Sn, i.e., when the 1f7/2 orbital is completely filled, had been proposed in the past, in analogy to the magicity of 48Ca, featuring a completely filled 0f7/2 orbital one harmonic oscillator shell below.
U2 - 10.1016/j.physletb.2024.138561
DO - 10.1016/j.physletb.2024.138561
M3 - Article
SN - 0370-2693
VL - 851
JO - Physics Letters B
JF - Physics Letters B
M1 - 138561
ER -