14N(3He,d)15O as a probe of direct capture in the 14N(p,γ)15O reaction

P. F. Bertone, A. E. Champagne, M. Boswell, C. Iliadis, S. E. Hale, V. Y. Hansper, and D. C. Powell
Phys. Rev. C 66, 055804 – Published 27 November 2002
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Abstract

Spectroscopic factors and asymptotic normalization coefficients (ANCs) have been determined for bound states in 15O using the 14N(3He,d)15O reaction. These results are used to calculate the astrophysical S factor for direct capture in the 14N(p,γ)15O reaction. We also discuss how uncertainties in optical-model parameters influence both the spectroscopic factors and the ANCs, and the effect that this has on the predicted direct-capture reaction rate.

  • Received 12 July 2002

DOI:https://doi.org/10.1103/PhysRevC.66.055804

©2002 American Physical Society

Authors & Affiliations

P. F. Bertone, A. E. Champagne, M. Boswell, C. Iliadis, S. E. Hale, V. Y. Hansper, and D. C. Powell

  • University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599-3255
  • Triangle Universities Nuclear Laboratory, Durham, North Carolina 27708-0308

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Vol. 66, Iss. 5 — November 2002

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