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) | 
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
	
	
	