Tipus de document

Article

Versió

Versió publicada

Data de publicació

Llicència de publicació

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

Títol de la revista

Director/Tutor

ISSN de la revista

Títol del volum

Resum

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.

Matèries (anglès)

Citació

Citació

SEASTAR Collaboration, et al. Shell evolution of N = 40 isotones towards 60Ca: First spectroscopy of 62Ti. Physics Letters B. 2019. Vol. 800, num. 135071. ISSN 0370-2693. [consulted: 9 of September of 2026]. Available at: https://hdl.handle.net/2445/215202

Exportar metadades

JSON - METS

Compartir registre