Decay of the double--K-shell-vacancy state in silver atoms created in the decay of 109Cd

A pair of germanium detectors and a three-parameter analyzer were applied in an experimental study of the creation and of the decay of atomic states with a double K-shell vacancy, created in the decay of 109Cd. Assuming a variable intensity ratio of the Kα1 and Kα2 hypersatellite lines, their shift with respect to the diagram lines, Δ/sub K/α/sup h/ = 546 +- 20 eV, and the shift of the Kα satellite lines with an initial L-shell vacancy, Δ/sub K/α/sup s/(L-1) = 54 +- 6 eV, were obtained. The former result is in agreement with the previous experimental result of van Eijk et al. and with the theoretical result of Chen et al., but the latter result is significantly lower than the theoretical value of 73 eV. For the I(Kα1 /sup h/)/I(Kα/sup h/) intensity ratio, a value of 0.54 +- 0.11 was obtained. From the numbers of counts in the hypersatellite-satellite peaks the intensity ratios of the hypersatellite lines I(Kβ/sub 1prime/ /sup h/)/I(Kα/sup h/) = 0.195 +- 0.016, and I(Kβ/sub 2prime/ /sup h/)/I(Kα/sup h/) = 0.055 +- 0.008 were obtained. The former value seems to be larger than the theoretical value 0.168, while the latter value is significantly larger than the theoretical value 0.029