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Phys. Rev. C 80, 012801(R) (2009) [5 pages]

Improved determination of the astrophysical S(0) factor of the 15N(p,α)12C reaction

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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

Received 13 April 2009; revised 27 May 2009; published 13 July 2009

We present new improved R matrix fits of direct data and indirect Trojan Horse data for the 15N(p,α)12C 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.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.80.012801
DOI:
10.1103/PhysRevC.80.012801
PACS:
24.10.-i, 26.20.-f, 25.40.Hs, 27.20.+n