Abstract
The delayed neutron emitters and have been studied with a neutron detector and radiations have been measured with a Ge(Li) detector. was formed in the reaction (, ) with 56-MeV ions, and also in the reaction with 40-MeV ions. The thermalized neutrons following both reactions yield together a half-life of 0.747 ± 0.008 sec with the well-known 4.17-sec activity as an accompaniment formed in the (, ) and reactions. The neutron spectra in a bare detector contain lines of 0.79 ± 0.03 MeV and 1.72 ± 0.05 MeV with relative intensities in addition to peaks. The neutron groups are assigned to the decay to the known 3.36- and 4.32-MeV states of with branches of 84.4 ± 1.7% and 15.6 ± 1.7%, respectively.A search for rays associated with forbidden decay to the , , and levels of at 0.121, 0.297, and 0.397 MeV, respectively, gave upper limits of 0.5%, 0.5%, and 0.7% for the respective branching ratios (, respectively). The values for decay to the 3.36- and 4.32-MeV states, 3.551 ± 0.012 and 3.83 ± 0.05, respectively, compare with preliminary theoretical values of 6.49 and 3.94, respectively, due to Millener. Separate studies were made of decay, formed in the reaction at MeV. By using an empirical neutron efficiency function, established for the detector with the reaction, -ray branches of to the neutron-emitting states at 4.55, 5.38, and 5.94 MeV were found to be 39.2 ± 2.0%, 48.0 ± 1.5%, and 7.9 ± 0.3%, respectively, in disagreement with two previously reported measurements. -ray measurements on with a Ge(Li) detector yielded the following: ratio of -ray branching intensities ; corresponding to for this -ray branch, thereby more firmly fixing the spin as ; energy of second-excited state 3055.2 ± 0.3 keV; and ground-state -ray branch from the 3055.2-keV level < 1.5%. The mirror decays of the system are discussed. An incidental result is a half-life of 178.3 ± 0.4 msec for formed in the reaction with 20-40-MeV ions.
RADIOACTIVITY , ; measured , , , ; deduced , decay schemes; compared with theory. ; measured .
- Received 29 October 1975
DOI:https://doi.org/10.1103/PhysRevC.13.835
©1976 American Physical Society