Delayed Gamma Rays from Photofission of U238, U235, and Th232

R. B. Walton, R. E. Sund, E. Haddad, J. C. Young, and C. W. Cook
Phys. Rev. 134, B824 – Published 25 May 1964
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Abstract

Absolute delayed gamma-ray intensities from the photofission of U238, U235, and Th232 were measured as a function of time after bursts of fissions produced by the bombardment of samples with 20-MeV x rays from an electron linear accelerator. For all three target nuclei, components of short-lived gamma rays, which are attributed to the decay of isomers formed either in fission or, less likely, by other photoreactions, contributed markedly to the gamma-ray activity for times up to 800 μsec after the beam pulse. Beyond 800 μsec the gamma-ray activity decreased little for times up to about 101 sec. The gamma rays emitted in this interval, the "plateau" region, and at longer times are believed to follow beta decay of fission fragments. In the "plateau" region, the absolute intensities of gamma rays (Eγ>0.51 MeV) from the photofission of U238, U235, and Th232 are 0.70, 0.26, and 0.35 photons/fission-sec, respectively. After 0.1 sec the gamma-ray decay curves have the same shapes as those observed by other investigators in neutron fission of the same target nuclei, but the absolute intensity from photofission is approximately a factor of two less than that from neutron fission.

  • Received 1 November 1963

DOI:https://doi.org/10.1103/PhysRev.134.B824

©1964 American Physical Society

Authors & Affiliations

R. B. Walton, R. E. Sund, E. Haddad, and J. C. Young

  • General Atomic Division of General Dynamics Corporation, John Jay Hopkins Laboratory for Pure and Applied Science, San Diego, California

C. W. Cook*

  • North American Aviation Incorporated, El Segundo, California

  • *Work initiated while the author was at General Dynamics/Convair, San Diego, California.

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Issue

Vol. 134, Iss. 4B — May 1964

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