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cc-by (c)  SEASTAR Collaboration et al., 2019
Si us plau utilitzeu sempre aquest identificador per citar o enllaçar aquest document: https://hdl.handle.net/2445/215202

Shell evolution of N = 40 isotones towards 60Ca: First spectroscopy of 62Ti

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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.

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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.. Shell evolution of N = 40 isotones towards 60Ca: First spectroscopy of 62Ti. _Physics Letters B_. 2019. Vol. 800, núm. 135071. [consulta: 30 de gener de 2026]. ISSN: 0370-2693. [Disponible a: https://hdl.handle.net/2445/215202]

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