Production of Th229 for medical applications: Excitation functions of low-energy protons on Th232 targets

J. R. Griswold, C. U. Jost, D. W. Stracener, S. H. Bruffey, D. Denton, M. Garland, L. Heilbronn, and S. Mirzadeh
Phys. Rev. C 98, 044607 – Published 12 October 2018
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Abstract

As a part of a general program to evaluate production routes for Th229, we studied production of Th229 via proton-induced reactions on Th232 targets bombarded with low-energy protons, Ep40MeV. The reported excitation functions include those for proton-induced reactions on natural thorium yielding to Pa228,229,230&232 isotopes; Th232(p,xn) reactions, where x=1, 3, 4, and 5, at proton energy ranges of 12–40 MeV. Although the data for Th232(p,n)Pa228, Th232(p,3n)Pa230, and Th232(p,5n)Pa232 reactions were deduced by direct analysis of the thorium foils after irradiation, the data for Th232(p,4n)Pa229 were obtained by radiochemical techniques. The half-life of Pa229 was evaluated and determined to be 1.55 ± 0.01 d. Further, the α-branching ratio, α/(α + EC) of Pa229 was evaluated to be 0.53 ± 0.10% by allowing Pa229 to decay for 7d, then chemically extracting and quantifying the Ac225 (t1/2=10.0±0.1d) from Pa229 samples. In addition, we report the effective production cross section of Th229 in a thick Th232 target in the proton energy range of 23–33 MeV. The peak of the excitation function for the Th232(p,4n)Pa229 reaction occurs at 162 ± 14 mb and Ep=29.7±0.5MeV. This is only slightly larger than the effective cross section for the Th232(p,x)Th229 reaction (obtained from a thick target experiment). This data indicates that the Th232(p,4n)Pa229 reaction is the major reaction pathway for the cumulative Th232(p,x)Th229 reaction cross section in this energy range. The measured cross sections were compared with theoretical cross sections using the simulation codes Particle and Heavy Ion Transport code System (PHITS) and Monte Carlo Neutral Particle 6 (MCNP6). At proton energy ranges of 12–33 MeV, the cumulative excitation function predicted by PHITS for the reactions leading to Th229 was in close agreement with the experimental function, whereas the function predicted by MCNP6 was a factor of two higher at the peak of the excitation function.

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  • Received 5 February 2018

DOI:https://doi.org/10.1103/PhysRevC.98.044607

©2018 American Physical Society

Physics Subject Headings (PhySH)

Accelerators & BeamsNuclear Physics

Authors & Affiliations

J. R. Griswold1,2, C. U. Jost3,4, D. W. Stracener3, S. H. Bruffey1, D. Denton1, M. Garland1,*, L. Heilbronn2, and S. Mirzadeh1

  • 1Nuclear Security and Isotope Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 2Department of Nuclear Engineering, University of Tennessee, Knoxville, Tennessee 37996, USA
  • 3Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 4Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA

  • *Present address: Department of Energy, Office of Nuclear Physics, Isotope Program, SC-26/Germantown Building, 1000 Independence Ave., SW, Washington, DC 20585, USA.

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Issue

Vol. 98, Iss. 4 — October 2018

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