Please use this identifier to cite or link to this item:
https://hdl.handle.net/2445/215202
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | SEASTAR Collaboration | - |
dc.contributor.author | Holt, J.D. | - |
dc.contributor.author | Lenzi, S.M. | - |
dc.contributor.author | Menéndez Sánchez, Javier | - |
dc.contributor.author | Nowacki, F. | - |
dc.contributor.author | Ogata, K. | - |
dc.contributor.author | Poves, A. | - |
dc.contributor.author | Rodríguez, T.R. | - |
dc.contributor.author | Schwenk, A. | - |
dc.contributor.author | Simonis, J. | - |
dc.contributor.author | Stroberg, S.R. | - |
dc.contributor.author | Yoshida, K. | - |
dc.date.accessioned | 2024-09-17T09:32:44Z | - |
dc.date.available | 2024-09-17T09:32:44Z | - |
dc.date.issued | 2019-11-04 | - |
dc.identifier.issn | 0370-2693 | - |
dc.identifier.uri | https://hdl.handle.net/2445/215202 | - |
dc.description.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. | - |
dc.format.extent | 1 p. | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | - |
dc.publisher | Elsevier B.V. | - |
dc.relation.isformatof | Reproducció del document publicat a: https://doi.org/10.1016/j.physletb.2019.135071 | - |
dc.relation.ispartof | Physics Letters B, 2019, vol. 800, p. 135071 | - |
dc.relation.uri | https://doi.org/10.1016/j.physletb.2019.135071 | - |
dc.rights | cc-by (c) SEASTAR Collaboration et al., 2019 | - |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | - |
dc.source | Articles publicats en revistes (Física Quàntica i Astrofísica) | - |
dc.subject.classification | Isòtops | - |
dc.subject.classification | Espectrometria de raigs gamma | - |
dc.subject.other | Isotopes | - |
dc.subject.other | Gamma ray spectrometry | - |
dc.title | Shell evolution of N = 40 isotones towards 60Ca: First spectroscopy of 62Ti | - |
dc.type | info:eu-repo/semantics/article | - |
dc.type | info:eu-repo/semantics/publishedVersion | - |
dc.identifier.idgrec | 697630 | - |
dc.date.updated | 2024-09-17T09:32:44Z | - |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | - |
Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
225558.pdf | 1.04 MB | Adobe PDF | View/Open |
This item is licensed under a
Creative Commons License