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The Disintegration of Sr91 and Y91m

D. P. Ames*, M. E. Bunker, L. M. Langer, and B. M. Sorenson

  • University of California, Los Alamos Scientific Laboratory, Los Alamos, New Mexico

  • *Now at the University of Kentucky, Lexington, Kentucky.
  • Indiana University, Bloomington, Indiana.

Phys. Rev. 91, 68 – Published 1 July, 1953

DOI: https://doi.org/10.1103/PhysRev.91.68

Abstract

The radiations from the fission product Sr91 (9.67-hr) and its daughter isomer Y91m (50.3-min) have been studied using a magnetic lens spectrometer, a high resolution 180° focusing spectrometer, and a scintillation spectrometer. Coincidence measurements were made to check on certain genetic aspects of the decay scheme. Five beta-ray groups are observed with end-point energies and relative intensities of 2.665 Mev, 26.4 percent; 2.03 Mev, 4.1 percent; 1.359 Mev, 29.2 percent; 1.093 Mev, 33.1 percent; and 0.62 Mev, 7.2 percent. The 2.665-Mev group has a shape characteristic of a once forbidden transition involving a spin change of 2 units. Gamma-rays are found with energies of 1.413, 1.025, 0.93, 0.748, 0.645, and 0.5512 Mev. The 50.3-min isomeric level in Y91 decays only by gamma-emission to the ground state. The 0.5512-Mev gamma-ray associated with this transition has a K(L+M) internal conversion ratio of 6.00, which is consistent with an M4 assignment. A disintegration scheme is proposed.

References (13)

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