Determining the 239Np(n,f) cross section using the surrogate ratio method

A. Czeszumska, C. T. Angell, J. T. Harke, N. D. Scielzo, E. B. Norman, R. A. E. Austin, G. Boutoux, R. J. Casperson, P. Chodash, R. O. Hughes, C. M. Mattoon, V. Méot, J. Munson, L. Phair, J. J. Ressler, O. Roig, T. J. Ross, E. Swanberg, and B. Wang
Phys. Rev. C 87, 034613 – Published 12 March 2013

Abstract

Background: Neutron-induced fission cross-section data are needed in various fields of applied and basic nuclear science. However, cross sections of short-lived nuclei are difficult to measure directly due to experimental constraints.

Purpose: The first experimental determination of the neutron-induced fission cross section of 239Np at nonthermal energies was performed. This minor actinide is the waiting point to 240Pu production in a nuclear reactor.

Method: The surrogate ratio method was employed to indirectly deduce the 239Np(n,f) cross section. The surrogate reactions used were 236U(3He,p) and 238U(3He,p) with the reference cross section given by the well-known 237Np(n,f) cross section. The ratio of observed fission reactions resulting from the two formed compound nuclei, 238Np and 240Np, was multiplied by the directly measured 237Np(n,f) cross section to determine the 239Np(n,f) cross section.

Results: The 239Np(n,f) cross section was determined with an uncertainty ranging between 4% and 30% over the energy range of 0.5–20 MeV. The resulting cross section agrees closest with the JENDL-4.0 evaluation.

Conclusions: The measured cross section falls in between the existing evaluations, but it does not match any evaluation exactly (with JENDL-4.0 being the closest match); hence reactor codes relying on existing evaluations may under- or overestimate the amount of 240Pu produced during fuel burnup. The measurement helps constrain nuclear structure parameters used in the evaluations.

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  • Received 23 December 2012

DOI:https://doi.org/10.1103/PhysRevC.87.034613

©2013 American Physical Society

Authors & Affiliations

A. Czeszumska1,*, C. T. Angell1,2, J. T. Harke3, N. D. Scielzo3, E. B. Norman1,3,4, R. A. E. Austin5, G. Boutoux6,7, R. J. Casperson3, P. Chodash1, R. O. Hughes8, C. M. Mattoon3, V. Méot9, J. Munson1, L. Phair4, J. J. Ressler3, O. Roig9, T. J. Ross8,10, E. Swanberg1, and B. Wang1

  • 1Department of Nuclear Engineering, University of California, Berkeley, California 94720, USA
  • 2Quantum Beam Science Directorate, Japan Atomic Energy Agency, Tokai-mura, Ibaraki 319-1195, Japan
  • 3Physics Division, Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 4Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 5Saint Mary's University, Halifax, Canada
  • 6CNRS, IN2P3, CENBG, UMR 5797, F-33175 Gradignan, France
  • 7Université de Bordeaux, CENBG, UMR 5797, F-33175 Gradignan, France
  • 8Department of Physics, University of Richmond, Richmond, Virginia 23173, USA
  • 9CEA DAM DIF, F-91297 Arpajon, France
  • 10Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom

  • *agac@berkeley.edu

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Issue

Vol. 87, Iss. 3 — March 2013

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