High-precision branching ratio measurement for the superallowed β+ emitter Ga62

P. Finlay, G. C. Ball, J. R. Leslie, C. E. Svensson, I. S. Towner, R. A. E. Austin, D. Bandyopadhyay, A. Chaffey, R. S. Chakrawarthy, P. E. Garrett, G. F. Grinyer, G. Hackman, B. Hyland, R. Kanungo, K. G. Leach, C. M. Mattoon, A. C. Morton, C. J. Pearson, A. A. Phillips, J. J. Ressler, F. Sarazin, H. Savajols, M. A. Schumaker, and J. Wong
Phys. Rev. C 78, 025502 – Published 19 August 2008

Abstract

A high-precision branching ratio measurement for the superallowed β+ decay of Ga62 was performed at the Isotope Separator and Accelerator (ISAC) radioactive ion beam facility. The 8π spectrometer, an array of 20 high-purity germanium detectors, was employed to detect the γ rays emitted following Gamow-Teller and nonanalog Fermi β+ decays of Ga62, and the SCEPTAR plastic scintillator array was used to detect the emitted β particles. Thirty γ rays were identified following Ga62 decay, establishing the superallowed branching ratio to be 99.858(8)%. Combined with the world-average half-life and a recent high-precision Q-value measurement for Ga62, this branching ratio yields an ft value of 3074.3±1.1 s, making Ga62 among the most precisely determined superallowed ft values. Comparison between the superallowed ft value determined in this work and the world-average corrected Ft¯ value allows the large nuclear-structure-dependent correction for Ga62 decay to be experimentally determined from the CVC hypothesis to better than 7% of its own value, the most precise experimental determination for any superallowed emitter. These results provide a benchmark for the refinement of the theoretical description of isospin-symmetry breaking in A62 superallowed decays.

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  • Received 25 April 2008

DOI:https://doi.org/10.1103/PhysRevC.78.025502

©2008 American Physical Society

Authors & Affiliations

P. Finlay1,*, G. C. Ball2, J. R. Leslie3, C. E. Svensson1, I. S. Towner3, R. A. E. Austin4, D. Bandyopadhyay1, A. Chaffey4, R. S. Chakrawarthy2, P. E. Garrett1,2, G. F. Grinyer1,†, G. Hackman2, B. Hyland1, R. Kanungo2,‡, K. G. Leach1, C. M. Mattoon5, A. C. Morton2, C. J. Pearson2, A. A. Phillips1, J. J. Ressler6, F. Sarazin5, H. Savajols2, M. A. Schumaker1, and J. Wong1

  • 1Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
  • 2TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
  • 3Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
  • 4Department of Astronomy and Physics, Saint Mary's University, Halifax, Nova Scotia B3H 3C3, Canada
  • 5Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA
  • 6Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada

  • *pfinlay@physics.uoguelph.ca.
  • Present address: National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Present address: Department of Astronomy and Physics, St. Mary's University, Halifax, Nova Scotia B3H 3C3, Canada.

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Vol. 78, Iss. 2 — August 2008

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