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Improved determination of the astrophysical S(0) factor of the N15(p,α)C12 reaction

M. La Cognata, V. Z. Goldberg, A. M. Mukhamedzhanov, C. Spitaleri, and R. E. Tribble
Phys. Rev. C 80, 012801(R) – Published 13 July 2009

Abstract

We present new improved R matrix fits of direct data and indirect Trojan Horse data for the N15(p,α)C12 reaction and provide a more accurate recommended value of S(0)=73.0±5.0 MeV b from direct Redder data [A. Redder et al., Z. Phys. A 305, 325 (1982)] and S(0)=70.0±13.5 MeV b from the Trojan Horse data [M. La Cognata et al., Phys. Rev. C 76, 065804 (2007)]. We also analyze a recent fit by Barker [F. C. Barker, Phys. Rev. C 78, 044611 (2008)] and demonstrate that when all the uncertainties are taken into account, our results overlap with his. We also provide a fit of the Trojan Horse data that properly takes into account finite residual energy resolution of the data.

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  • Received 13 April 2009

DOI:https://doi.org/10.1103/PhysRevC.80.012801

©2009 American Physical Society

Authors & Affiliations

M. La Cognata1, V. Z. Goldberg2, A. M. Mukhamedzhanov2, C. Spitaleri1,*, and R. E. Tribble2

  • 1DMFCI, Università di Catania, Catania, Italy and INFN-Laboratori Nazionali del Sud, Catania, Italy
  • 2Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA

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Vol. 80, Iss. 1 — July 2009

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