Induced Radioactivity in Strontium and Yttrium; Nuclear Isomers in Strontium

David W. Stewart
Phys. Rev. 56, 629 – Published 1 October 1939
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Abstract

In revising and extending previous work on induced radioactivity in strontium and yttrium, it was found that with stronger activation by deuterons and neutrons, more accurate determinations could be made of the radioactive decay periods, and measurements of beta- and gamma-ray energies could be made with greater certainty. Periods of 2.0±0.2 hours, 14±2 hours, and 82±4 hours were found in yttrium separated from strontium bombarded with 7-Mev deuterons. The first of these periods was assigned to Y88, and the other two either to Y85 and Y87, or to isomeric forms of either of these. Periods of 3.0±0.1 hours and 55±5 days, produced in strontium by bombardment of that element with deuterons and neutrons, were assigned to the decay of isomeric forms of Sr89, and the nature of that isomerism was investigated. From measurements in the cloud chamber, the maximum energy of the beta-rays from the 3-hour isomer was found to be 0.60 Mev, those from the 55-day isomer had an upper limit of 1.50 Mev, and the gamma-radiation which accompanied the 3-hour decay was found to have two components, of 0.55 Mev and 1.10 Mev. A tentative energy level diagram suggests that the metastable state of Sr89 decays first by the emission of a beta-particle and then by the emission of either one or two gamma-rays. The ground state of Sr89 decays directly to the ground state of Y89 without the emission of gamma-radiation.

  • Received 16 August 1939

DOI:https://doi.org/10.1103/PhysRev.56.629

©1939 American Physical Society

Authors & Affiliations

David W. Stewart*

  • Departments of Chemistry and Physics, University of Michigan, Ann Arbor, Michigan

  • *Present address, Department of Chemistry, Columbia University, New York.

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Issue

Vol. 56, Iss. 7 — October 1939

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