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

dc.contributor.authorSEASTAR Collaboration
dc.contributor.authorHolt, J.D.
dc.contributor.authorLenzi, S.M.
dc.contributor.authorMenéndez Sánchez, Javier
dc.contributor.authorNowacki, F.
dc.contributor.authorOgata, K.
dc.contributor.authorPoves, A.
dc.contributor.authorRodríguez, T.R.
dc.contributor.authorSchwenk, A.
dc.contributor.authorSimonis, J.
dc.contributor.authorStroberg, S.R.
dc.contributor.authorYoshida, K.
dc.date.accessioned2024-09-17T09:32:44Z
dc.date.available2024-09-17T09:32:44Z
dc.date.issued2019-11-04
dc.date.updated2024-09-17T09:32:44Z
dc.description.abstractExcited 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.
dc.format.extent1 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec697630
dc.identifier.issn0370-2693
dc.identifier.urihttps://hdl.handle.net/2445/215202
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1016/j.physletb.2019.135071
dc.relation.ispartofPhysics Letters B, 2019, vol. 800, p. 135071
dc.relation.urihttps://doi.org/10.1016/j.physletb.2019.135071
dc.rightscc-by (c) SEASTAR Collaboration et al., 2019
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationIsòtops
dc.subject.classificationEspectrometria de raigs gamma
dc.subject.otherIsotopes
dc.subject.otherGamma ray spectrometry
dc.titleShell evolution of N = 40 isotones towards 60Ca: First spectroscopy of 62Ti
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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