Abstract

A new decay scheme is given for ${\mathrm{Cu}}^{60}$ which agrees with the main features of previous schemes. However, evidence was found for previously unreported feedings to levels at 4.08, 3.73, 3.39, 3.27, and 3.19 MeV. Analysis of single-crystal $\ensuremath{\gamma}$-ray spectra and spectra in coincidence with 1.33-MeV radiation and with annihilation radiation revealed, in addition to previously established $\ensuremath{\gamma}$ rays, new weaker $\ensuremath{\gamma}$ rays whose energies are 0.47, 0.50, 0.64, 0.95, 1.03, (1.10), 1.86, 1.94, 2.06, 2.40, 2.74, 3.19, and 3.27 MeV. No 3.52-MeV $\ensuremath{\gamma}$ ray was found. The half-life for ${\mathrm{Cu}}^{60}$ was measured to be 22.9\ifmmode\pm\else\textpm\fi{}0.1 min. Angular-correlation measurements for $\ensuremath{\gamma}$ rays of 0.83, 0.95, 1.03, and 1.79 MeV in coincidence with 1.33-MeV radiation have been made. Spin-2 assignments resulted for levels at 2.16 and 3.12 MeV. $\frac{E2}{M1}$ mixing ratios $\ensuremath{\delta}=\ensuremath{-}1.2\ifmmode\pm\else\textpm\fi{}0.3 \mathrm{and} 0.21\ifmmode\pm\else\textpm\fi{}0.04$ were found for ${{2}_{i}}^{+}\ensuremath{\rightarrow}{{2}_{1}}^{+}$ transitions of 0.83 and 1.79 MeV, respectively. A spin-0 assignment for the 2.29-MeV level was made. The present $\ensuremath{\gamma}\ensuremath{-}\ensuremath{\gamma}$ angular-correlation results are compared with results of a previous $\ensuremath{\gamma}\ensuremath{-}\ensuremath{\gamma}$ angular-correlation study and with results of a ${\mathrm{Ni}}^{60}(p, {p}^{\ensuremath{'}}\ensuremath{\gamma})$ $\ensuremath{\gamma}$-ray angular-distribution study. In the case of the $\frac{E2}{M1}$ mixing ratio for the 0.83-MeV $\ensuremath{\gamma}$ ray arising from the 2.16-MeV level, the present value for $\ensuremath{\delta}$ is close to the value obtained from the ($p, {p}^{\ensuremath{'}}\ensuremath{\gamma}$) study, and disagrees with the previous radioactivity work. The negative sign of $\ensuremath{\delta}$ for this ${2}_{2}^{+}$\ensuremath{\rightarrow}${2}_{1}^{+}$ transition is discussed in the light of new theoretical estimates by Greiner. The relationship of the present experiment to other recent work is discussed.

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