Ratio of S factors for (p,γ) reactions on 12C and 13C at astrophysically relevant energies

C. D. Nesaraja, C. R. Brune, B. T. Crowley, J. H. Kelley, S. O. Nelson, R. M. Prior, K. Sabourov, D. R. Tilley, A. Tonchev, and H. R. Weller
Phys. Rev. C 64, 065804 – Published 21 November 2001
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Abstract

We present measurements of the 12C(p,γ0)13N/13C(p,γ0)14N S factor ratio at Ep=160keV. The overall result of 0.33±0.03 is in good agreement with the value of this ratio obtained from previous experimental values of the S factors for the 12C(p,γ0)13N and the 13C(p,γ0)14N reactions. A value for the total S factor ratio of S[12C(p,γtotal)]/S[13C(p,γtotal)]=0.24±0.03 is computed by correcting the 13C(p,γ0) S factor for transitions to the other intermediate states. The direct + resonance model calculation of this ratio and the impact on the CNO cycle are also explored.

  • Received 19 July 2001

DOI:https://doi.org/10.1103/PhysRevC.64.065804

©2001 American Physical Society

Authors & Affiliations

C. D. Nesaraja1,2, C. R. Brune2,4, B. T. Crowley1,2, J. H. Kelley2,3, S. O. Nelson1,2, R. M. Prior2,5, K. Sabourov1,2, D. R. Tilley2,3, A. Tonchev1,2, and H. R. Weller1,2

  • 1Duke University, Durham, North Carolina 27708
  • 2Triangle Universities Nuclear Laboratory, Durham, North Carolina 27708
  • 3North Carolina State University, Raleigh, North Carolina 27695
  • 4The University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599
  • 5North Georgia College and State University, Dahlonega, Georgia 30597

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Vol. 64, Iss. 6 — December 2001

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