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Yrast structure of neutron-rich {sup 53}Ti

Journal Article · · Physical Review. C, Nuclear Physics
; ; ;  [1]; ; ; ; ; ; ; ; ;  [2];  [3];  [4];  [2];  [5];  [1]; ;  [4]
  1. Institute of Nuclear Physics, Polish Academy of Sciences, PL-31342 Cracow (Poland)
  2. Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
  3. Center for Mathematical Sciences, University of Aizu, Tsuruga, Ikki-machi, Aizu-Wakamatsu, Fukushima 965-8580 (Japan)
  4. National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824 (United States)
  5. Nuclear Engineering Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
{gamma} rays from neutron-rich Ti nuclei in the vicinity of N=32 have been studied at Gammasphere using deep-inelastic reactions induced by {sup 48}Ca beams on thick {sup 208}Pb and {sup 238}U targets. The {sup 53}Ti yrast cascade was identified for the first time, and the location in energy of states with spin up to I = 21/2 was determined. The excitations of {sup 53}Ti provide new tests of effective interactions for full-pf-shell calculations. Comparisons between theory and experiment for the highest spin states in {sup 53}Ti favor the recently proposed GXPF1A interaction, which accounts for the appearance of a neutron subshell closure at N=32 in Ti isotopes as well as for the lack of a similar subshell closure at N=34, as predicted by earlier calculations with another interaction.
OSTI ID:
20699061
Journal Information:
Physical Review. C, Nuclear Physics, Journal Name: Physical Review. C, Nuclear Physics Journal Issue: 4 Vol. 72; ISSN 0556-2813; ISSN PRVCAN
Country of Publication:
United States
Language:
English