Positron Emission fromAg105and Related Aspects ofAg105Decay

Abstract
Positron emission in the decay of 40-day Ag105 has been discovered by detection of the 180°-coincident annihilation γ rays. The intensity is 8.6±1.4 positrons per million Ag105 disintegrations. Of these, only about (2±2)% can be attributed to processes associated with γ transitions, leaving 8.5±1.5 positrons per million disintegrations attributable only to positron emission as a mode of β decay of Ag105. By γγγ triple-coincidence measurements, it was found that these positrons (or the bulk of them) are not in coincidence with γ rays, and hence that the transition is probably between the Ag105 and Pd105 ground states. The spectrum of the positrons was obtained by βγγ triple-coincidence measurements, and it was found to have an endpoint of 325±25 keV. The implied logf1t value (8.5) is within the range predicted for the expected but hitherto-undocumented unique first-forbidden transition between the Ag105 and Pd105 ground states, the spins and parities of both of which are known (1252+). Radiations observed by means of NaI(Tl), Ge(Li), and Si(Li) spectrometry were the Pd K x rays (abundance 78% of the Ag105 disintegrations) and the following γ rays: 64.07 (11%), 155 (0.5%), 182.7 (0.5%), 280.5 (32%), 306.3 (0.7%), 319.4 (4%), 331.6 (4%), 344.5 (42%), 360.7 (0.6%), 370.2 (0.7%), 392.8 (2%), 415.5 (0.2%), 443.4 (11%), 526.4 (0.09%), 560.4 (0.5%), 617.8 (1%), 644.4 (10%), 649.6 (3%), 673.2 (0.9%), 726.3 (0.2%), 743.1 (0.5%), 807.3 (1%), 961.5 (0.1%), and 1087.8 (4%) keV. By x-γ coincidence measurements, it was shown that the lifetime of the 344-keV level of Pd105 is short (t12<6×108 sec), in contradiction to recent assertions. The