β-delayed neutron spectroscopy of Co70,72 ground-state and isomeric-state decays

  • K. Siegl
  • , A. M. Keeler
  • , R. Grzywacz
  • , N. T. Brewer
  • , B. P. Crider
  • , A. Fijalkowska
  • , S. Go
  • , M. Hall
  • , J. H. Hamilton
  • , S. V. Ilyushkin
  • , T. King
  • , S. Liddick
  • , M. Madurga
  • , P. D. O'Malley
  • , S. V. Paulauskas
  • , M. M. Rajabali
  • , S. Z. Taylor
  • , E. H. Wang
  • , Z. Y. Xu
  • , C. Zachary

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

The β-decaying states of Co70,72 were studied at the National Superconducting Cyclotron Laboratory using the VANDLE neutron time-of-flight array. The (6-,7-)β-decaying state in Co70 is near-spherical with a lifetime of 113±7 ms, and the low-spin (1+,2+)β-decaying state is postulated to be the prolate deformed ground state with a lifetime of 508±7 ms. Both decay predominantly to the bound states of Ni70. For the first time neutron-emissions from neutron unbound states from both the (6-,7-) and (1+,2+)β decays were measured. Even with the low statistics data, we were able to disentangle the neutron emission from both decays, which enabled a determination of β-decay strength above the neutron separation energy of Ni70. Neutron emission probabilities were measured to be 7.1±1.5% and 9.4±1.7%, respectively, for the (6-,7-) and (1+,2+) decays. The decay pattern of the Co70 is driven by neutron f5/2 to proton f7/2 Gamow-Teller transformation. The observed population of neutron unbound states is attributed to the conversion of p1/2 and p3/2 neutrons to p3/2 and p1/2 protons excited across the Z=28 closed shell.

Original languageEnglish
Article number064309
JournalPhysical Review C
Volume109
Issue number6
DOIs
StatePublished - Jun 2024
Externally publishedYes

Funding

This research was sponsored in part by the Office of Nuclear Physics, U.S. Department of Energy under Awards No. DE-FG02-96ER40983 (UTK) and No. DE-AC05-00OR22725 (ORNL), and by the National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Awards No. DE-NA0003899 and No. DE-NA0004068, U.S. Department of Energy, National Nuclear Security Administration, Grant No. DE-NA0004068, and National Science Foundation under Grant No. PHY 1848177 (CAREER) This research was sponsored in part by the Office of Nuclear Physics, U.S. Department of Energy under Awards No. DE-FG02-96ER40983 (UTK) and No. DE-AC05-00OR22725 (ORNL), and by the National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Awards No. DE-NA0003899 and No. DE-NA0004068, U.S. Department of Energy, National Nuclear Security Administration, Grant No. DE-NA0004068, and National Science Foundation under Grant No. PHY 1848177 (CAREER).

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