Identification of significant E0 strength in the 22+ → 21+ transitions of 58,60,62Ni

  • L. J. Evitts
  • , A. B. Garnsworthy
  • , T. Kibedi
  • , J. Smallcombe
  • , M. W. Reed
  • , B. A. Brown
  • , A. E. Stuchbery
  • , G. J. Lane
  • , T. K. Eriksen
  • , A. Akber
  • , B. Alshahrani
  • , M. de Vries
  • , M. S. M. Gerathy
  • , J. D. Holt
  • , B. Q. Lee
  • , B. P. McCormick
  • , A. J. Mitchell
  • , M. Moukaddam
  • , S. Mukhopadhyay
  • , N. Palalani
  • T. Palazzo, E. E. Peters, A. P. D. Ramirez, S. R. Stroberg, T. Tornyi, S. W. Yates

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Abstract

The E0 transition strength in the 22+ → 21transitions of 58,60,62Ni have been determined for the first time following a series of measurements at the Australian National University (ANU) and the University of Kentucky (UK). The CAESAR Compton-suppressed HPGe array and the Super-e solenoid at ANU were used to measure the δ(E2/M1) mixing ratio and internal conversion coefficient of each transition following inelastic proton scattering. Level half-lives, δ(E2/M1) mixing ratios and γ-ray branching ratios were measured at UK following inelastic neutron scattering. The new spectroscopic information was used to determine the E0 strengths. These are the first 22+ → 21+ E0 transition strengths measured in nuclei with spherical ground states and the E0 component is found to be unexpectedly large; in fact, these are amongst the largest E0 transition strengths in medium and heavy nuclei reported to date.
Original languageEnglish
JournalPhysics Letters B
Early online date21 Feb 2018
DOIs
Publication statusPublished - 10 Apr 2018
Externally publishedYes

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