| dc.creator | La Cognata, M. | |
| dc.creator | Goldberg, V. Z. | |
| dc.creator | Mukhamedzhanov, A. M. | |
| dc.creator | Spitaleri, C. | |
| dc.creator | Tribble, Robert E. | |
| dc.date.accessioned | 2011-09-13T21:26:07Z | |
| dc.date.available | 2011-09-13T21:26:07Z | |
| dc.date.issued | 2009 | |
| dc.identifier.citation | M. La Cognata, V. Z. Goldberg, A. M. Mukhamedzhanov, C. Spitaleri and Robert E. Tribble. Phys.Rev.C 80 012801 2009. "Copyright (2009) by the American Physical Society." | en |
| dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevC.80.012801 | |
| dc.identifier.uri | https://hdl.handle.net/1969.1/127082 | |
| dc.description | Journals published by the American Physical Society can be found at http://publish.aps.org/ | en |
| dc.description.abstract | We present new improved R matrix fits of direct data and indirect Trojan Horse data for the (15)N(p,alpha)(12)C reaction and provide a more accurate recommended value of S(0)=73.0 +/- 5.0 MeV b from direct Redder data [A. Redder , Z. Phys. A 305, 325 (1982)] and S(0)=70.0 +/- 13.5 MeV b from the Trojan Horse data [M. La Cognata , 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. | en |
| dc.language.iso | en | |
| dc.publisher | American Physical Society | |
| dc.subject | Physics | en |
| dc.title | Improved determination of the astrophysical S(0) factor of the (15)N(p,alpha)(12)C reaction | en |
| dc.type | Article | en |
| local.department | Physics and Astronomy | en |
