Measurement of the B10(α,n0)13N cross section for 2.2<Eα<4.9MeV and its application as a diagnostic at the National Ignition Facility

Q. Liu, M. Febbraro, R. J. deBoer, A. Boeltzig, Y. Chen, C. Cerjan, M. Couder, B. Frentz, J. Görres, E. A. Henry, E. Lamere, K. T. Macon, K. V. Manukyan, L. Morales, P. D. O'Malley, S. D. Pain, W. A. Peters, D. Schneider, C. Seymour, G. Seymour, E. Temanson, R. Toomey, B. Vande Kolk, J. Weaver, and M. Wiescher
Phys. Rev. C 100, 034601 – Published 3 September 2019
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Abstract

The National Ignition Facility (NIF) provides the opportunity to study nuclear reactions under controlled conditions at high temperatures and pressures at a level never before achieved. However, the timescale of the deuterium-tritium (DT) implosion is only a few nanoseconds, making data collection and diagnostics very challenging. One method that has been proposed for obtaining additional information about the conditions of the implosion is to activate a dopant material using the α particles produced from the DT fuel as a diagnostic. The yield of the activated material can give a measure of the mixing that occurs in the capsule. One of the reactions that has been proposed is B10(α,n)N13 as it produces a radioactive reactant product with a convenient half-life of 10min. Although this reaction has several advantages for the application at hand, it has not seen much study in the present literature, resulting in large uncertainties in the cross section. Furthermore, for the current application, the cross section must be well characterized. With this motivation, the B10(α,n)N13 cross section has been remeasured for 2.2<Eα<4.9MeV with the angle-integrated ground-state cross section reported for the first time. The present results, combined with previous measurements, allow for a determination of the cross section to a significantly higher degree of accuracy and precision than obtained previously and are shown to be consistent with thick-target measurements. Preliminary calculations are performed to test the feasibility of this reaction as a diagnostic for a NIF implosion.

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  • Received 17 June 2019

DOI:https://doi.org/10.1103/PhysRevC.100.034601

©2019 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Q. Liu1, M. Febbraro2, R. J. deBoer1, A. Boeltzig1,*, Y. Chen1, C. Cerjan3, M. Couder1, B. Frentz1, J. Görres1, E. A. Henry3, E. Lamere1,†, K. T. Macon1,4, K. V. Manukyan1, L. Morales1, P. D. O'Malley1, S. D. Pain2, W. A. Peters2, D. Schneider3, C. Seymour1, G. Seymour1,‡, E. Temanson2, R. Toomey5, B. Vande Kolk1, J. Weaver6, and M. Wiescher1

  • 1Department of Physics, The Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556, USA
  • 2Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830, USA
  • 3Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 4Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
  • 5Department of Physics and Astronomy, Rutgers University, New Brunswick, New Jersey 08901, USA
  • 6Material Measurement Laboratory, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA

  • *Present address: Gran Sasso National Laboratory, Via G. Acitelli 22, 67100 Assergi, Italy.
  • Present address: Department of Physics and Applied Physics, University of Massachusetts Lowell, Lowell Massachusetts 01854, USA.
  • Present address: Rutgers University, Piscataway, New Jersey 08854, USA.

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Issue

Vol. 100, Iss. 3 — September 2019

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