B10(α, n0)N13 and B10(α, pi)C13 for 2<Eα<8 MeV

Stephen J. Wilson
Phys. Rev. C 11, 1071 – Published 1 April 1975
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Abstract

We present simultaneously obtained data for the mirror reactions B10(α, n0)N13 and B10(α, p0)C13 and interpret the yield ratio with the formula of Barker and Mann. All but one of the isospin-mixed levels emit neutrons more copiously than protons, although we might expect about half of them to emit protons more copiously. We also present B10(α, pi)C13 cross sections for groups which leave C13 in the ½ ground state; and in the ½+ 3.086, 323.684, and 52+3.854 MeV excited states. We expanded the angular distributions in Legendre polynomials and fitted the coefficients at some of the resonances with compound nucleus scattering theory, obtaining spin-parity assignments: 1+ at Ex(N14)=13.16, 2 at 13.24, (2+, 2, 3+) at 13.67, and (1+, 1) at 13.76 MeV. As part of the calibration of the neutron spectrometer, we found the total He3(n, p)H3 cross section is 422±58 mb for 3.5 MeV neutrons. This value is about 20% lower than currently accepted values.

NUCLEAR REACTIONS B10(α, pi) i=0, 1, 2, 3 (α, n0) E=210 MeV; measured σ(E, θ); deduced N14 levels, J, π, isospin impurity. Enriched targets, resolution 50 keV, θ=10160°; Legendre polynomial expansion of σ(E, θ); absolute cross sections. Total σ for He3(n, p) at En=3.5 MeV.

  • Received 1 July 1974

DOI:https://doi.org/10.1103/PhysRevC.11.1071

©1975 American Physical Society

Authors & Affiliations

Stephen J. Wilson*,†

  • University of Wisconsin, Madison, Wisconsin 53706

  • *Present address: Physics Department, University of Guelph, Guelph, Ontario.
  • Work supported in part by the U. S. Atomic Energy Commission.

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Vol. 11, Iss. 4 — April 1975

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