Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/215202
Title: Shell evolution of N = 40 isotones towards 60Ca: First spectroscopy of 62Ti
Author: SEASTAR Collaboration
Holt, J.D.
Lenzi, S.M.
Menéndez Sánchez, Javier
Nowacki, F.
Ogata, K.
Poves, A.
Rodríguez, T.R.
Schwenk, A.
Simonis, J.
Stroberg, S.R.
Yoshida, K.
Keywords: Isòtops
Espectrometria de raigs gamma
Isotopes
Gamma ray spectrometry
Issue Date: 4-Nov-2019
Publisher: Elsevier B.V.
Abstract: Excited states in the isotone 62Ti were populated via the 63V62Ti reaction at ∼200 MeV/nucleon at the Radioactive Isotope Beam Factory and studied using γ-ray spectroscopy. The energies of the and transitions, observed here for the first time, indicate a deformed 62Ti ground state. These energies are increased compared to the neighboring 64Cr and 66Fe isotones, suggesting a small decrease of quadrupole collectivity. The present measurement is well reproduced by large-scale shell-model calculations based on effective interactions, while ab initio and beyond mean-field calculations do not yet reproduce our findings. The shell-model calculations for 62Ti show a dominant configuration with four neutrons excited across the gap. Likewise, they indicate that the island of inversion extends down to , disfavoring a possible doubly magic character of the elusive 60Ca.
Note: Reproducció del document publicat a: https://doi.org/10.1016/j.physletb.2019.135071
It is part of: Physics Letters B, 2019, vol. 800, p. 135071
URI: https://hdl.handle.net/2445/215202
Related resource: https://doi.org/10.1016/j.physletb.2019.135071
ISSN: 0370-2693
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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