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dc.creatorLa Cognata, M.en_US
dc.creatorRomano, S.en_US
dc.creatorSpitaleri, C.en_US
dc.creatorCherubini, S.en_US
dc.creatorCrucilla, V.en_US
dc.creatorGulino, M.en_US
dc.creatorLamia, L.en_US
dc.creatorPizzone, R. G.en_US
dc.creatorTumino, A.en_US
dc.creatorTribble, Robert E.en_US
dc.creatorFu, Changboen_US
dc.creatorGoldberg, V. Z.en_US
dc.creatorMukhamedzhanov, A. M.en_US
dc.creatorSchmidt, D.en_US
dc.creatorTabacaru, G.en_US
dc.creatorTrache, L.en_US
dc.creatorIrgaziev, B. F.en_US
dc.date.accessioned2011-09-13T21:27:16Z
dc.date.available2011-09-13T21:27:16Z
dc.date.issued2007en_US
dc.identifier.citationM. La Cognata, S. Romano, C. Spitaleri, S. Cherubini, V. Crucilla, M. Gulino, L. Lamia, R. G. Pizzone, A. Tumino, Robert E. Tribble, Changbo Fu, V. Z. Goldberg, A. M. Mukhamedzhanov, D. Schmidt, G. Tabacaru, L. Trache and B. F. Irgaziev. Phys.Rev.C 76 065804 2007. "Copyright (2007) by the American Physical Society."en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.76.065804en_US
dc.identifier.urihttp://hdl.handle.net/1969.1/127046
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en_US
dc.description.abstractThe low-energy bare-nucleus cross section for (15)N(p, alpha)(12)C is extracted by means of the Trojan horse method applied to the (2)H((15)N,alpha(12)C)n reaction at E(beam) = 60 MeV. For the first time we applied the modified half-off-energy-shell resonant R-matrix method that takes into account off-energy-shell effects and initial- and final-state interactions. In particular it has been shown that inclusion of Coulomb (15)N-d scattering and off-shell effects do not affect the determination of the astrophysical factor. Also the simple plane-wave approximation used in previous analyses is justified. The results extracted via the Trojan horse method are compared to direct data in the same energy region and show very good agreement in the energy interval 70-312 keV. These results confirm the extrapolations of the S factor reported in literature.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectASYMPTOTIC NORMALIZATION COEFFICIENTSen_US
dc.subjectQUASI-FREE SCATTERINGen_US
dc.subjectNUCLEARen_US
dc.subjectASTROPHYSICSen_US
dc.subjectSTELLAR ENERGIESen_US
dc.subjectCROSS-SECTIONSen_US
dc.subjectLIGHT-NUCLEIen_US
dc.subjectDISSOCIATIONen_US
dc.subjectRELEVANTen_US
dc.subjectCAPTUREen_US
dc.subjectLI-7(Pen_US
dc.subjectPhysicsen_US
dc.titleAstrophysical S(E) factor of the (15)N(p, alpha)(12)C reaction at sub-Coulomb energies via the Trojan horse methoden_US
dc.typeArticleen_US
local.departmentPhysics and Astronomyen_US


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