Abstract
The radiations from Rb84 have been investigated by means of scintillation coincidence spectrometer techniques in order to obtain the relative intensities of the various transitions. The energies and abundances of the radiations are 0.44-Mev β (5%), 0.81-Mev β+ (10%), 1.70-Mev β+ (9%), 0.89-Mev γ (64%), and 1.91-Mev γ (0.9%). [Note added in proof.—The β has been shown to be 0.91 Mev (2.5%).] Electron capture populates the level 1.91 Mev above the ground state, competes (54%) with the 0.81-Mev β+ to populate the level 0.89 Mev above ground, and competes (21%) with the 1.70-Mev β+ in effecting transitions to the ground state of Kr84. The ratios of K-capture to positron emission for the transition to the 0.89-Mev level (ΔI=0, yes) and to the Kr84 ground state (ΔI=2, yes) are 5.15±0.38 and 2.06±0.36, respectively. These values are in qualitative agreement with theory. Nucleon configurations of the several states of Rb84, Kr84, and Sr84 are discussed. In the decay to the 0.89-Mev level an LK-capture ratio of 0.12±0.05 was obtained by use of a value, 0.65, for the fluorescence yield of krypton. Alternatively, an experimental value for the fluorescence yield, 0.62±0.03, may be computed if the theoretical LK-capture ratio is assumed.