Remnants of spherical shell structures in deformed nuclei: The impact of an N=64 neutron subshell closure on the structure of N≈90 gadolinium nuclei

  • T. J. Ross
  • , R. O. Hughes
  • , C. W. Beausang
  • , J. M. Allmond
  • , C. T. Angell
  • , M. S. Basunia
  • , D. L. Bleuel
  • , J. T. Burke
  • , R. J. Casperson
  • , J. E. Escher
  • , P. Fallon
  • , R. Hatarik
  • , J. Munson
  • , S. Paschalis
  • , M. Petri
  • , L. W. Phair
  • , J. J. Ressler
  • , N. D. Scielzo

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

Abstract

Odd-mass gadolinium isotopes around N=90 were populated by the (p,d) reaction, utilizing 25-MeV protons, resulting in population of low-spin quasineutron states at energies near and below the Fermi surface. Systematics of the single quasineutron levels populated are presented. A large excitation energy gap is observed between levels originating from the 2d3/2, 1h11/2, and 3s1/2 spherical parents (above the N=64 gap), and the 2d5/2 (below the gap), indicating that the spherical shell model level spacing is maintained at least to moderate deformations.

Original languageEnglish
Article number031301
JournalPhysical Review C - Nuclear Physics
Volume88
Issue number3
DOIs
StatePublished - Sep 3 2013

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