2017
DOI: 10.1103/physrevc.96.024315
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High-spin states and lifetimes in S33 and shell-model interpretation in the sdfp space

Abstract: The structure of the 33 S nucleus was investigated in the 24 Mg(14 N,αp) fusion-evaporation reaction using a 40-MeV 14 N beam. The level scheme was extended up to an excitation energy of 11.7 MeV and spin 19/2 +. Lifetimes of the intermediate-and high-spin states have been investigated by the Doppler shift attenuation method. Data were compared with different shell-model calculations where effective interactions involving two main shells, the sd and the fp, are used.

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Cited by 5 publications
(4 citation statements)
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“…The wave function of the ground state has been calculated with 16 O core, where a good agreement has been found with experimental data for a positiveparity state using USDB as in [24]. The comparisons between experimental and calculated result are shown in Fig.…”
Section: Energy Levelssupporting
confidence: 55%
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“…The wave function of the ground state has been calculated with 16 O core, where a good agreement has been found with experimental data for a positiveparity state using USDB as in [24]. The comparisons between experimental and calculated result are shown in Fig.…”
Section: Energy Levelssupporting
confidence: 55%
“…Studying the excited states of this nucleus with the use of the shell model clarifies the various configurations of nucleons in the main valence shell for the positive-parity states, and the intruder excitations of the negative-parity states with crossshell configurations in or/and shells. The negative-parity states, named intruder states, accrue due to the promotion of one nucleon from the to shell for nuclei near 16 O, or from to shell for nuclei close to 40 Ca [10]. 24 Mg nucleus is po-sitioned in the middle of the shell, where there is a competition between the two types of transitions.…”
Section: Introductionmentioning
confidence: 99%
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“…For example, states of 35 S have recently been studied to spin (21/2 h) through the use of the 26 Mg( 18 O, 2α1n) 35 S reaction; in this case the physics interest centered around a comparison of the experimental level scheme with that predicted in state-of-the-art large-scale shell-model calculations using the SDPF_ MSD4 interaction [18]. Similarly, high-spin states and lifetimes in 33 S have been studied using the 24 Mg( 14 N, αp) reaction [19] and the results interpreted using shell-model calculations in the sd-f p space. On a completely different physics topic, the fundamental property of isospin symmetry of the nuclear interaction has been studied in the high-spin spectroscopy of the neutron-deficient 31 S nucleus and its mirror nucleus 31 P [20][21][22].…”
Section: Introductionmentioning
confidence: 99%