Benchmarking the external surrogate ratio method using the (α, α′f) reaction at STARS

  • S. R. Lesher
  • , L. A. Bernstein
  • , H. Ai
  • , C. W. Beausang
  • , D. Bleuel
  • , J. T. Burke
  • , R. M. Clark
  • , P. Fallon
  • , J. Gibelin
  • , I. Y. Lee
  • , B. F. Lyles
  • , A. O. Macchiavelli
  • , M. A. McMahan
  • , K. J. Moody
  • , E. B. Norman
  • , L. Phair
  • , E. Rodriguez-Vieitez
  • , M. Wiedeking

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We measured the ratio of the fission probabilities of 234U* relative to 236U* formed via an (α, α′) direct reactions using the STARS array at the 88-inch cyclotron at the Lawrence Berkeley National Laboratory. This ratio has a shape similar to the ratio of neutron capture probabilities from 233U(n,f) and 235U(n,f), indicating the alpha reactions likely formed a compound nucleus. This result indicates that the ratios of fission exit channel probabilities for two actinide nuclei populated via (α, α′) can be used to determine an unknown fission cross section relative to a known one. The validity of the External Surrogate Ratio Method (ESRM) is tested and the results support the conclusions of Burke et al. [1]. © 2008 American Institute of Physics.
Original languageEnglish
Title of host publication2007 International Workshop on Compound-Nuclear Reactions and Related Topics, CNR 2007
DOIs
StatePublished - 2008

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