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dc.creatorTrache, L.
dc.creatorAzhari, A.
dc.creatorClark, HL
dc.creatorGagliardi, Carl A.
dc.creatorLui, YW
dc.creatorMukhamedzhanov, AM
dc.creatorTribble, Robert E.
dc.creatorCarstoiu, F.
dc.date.accessioned2011-09-13T21:27:52Z
dc.date.available2011-09-13T21:27:52Z
dc.date.issued1998
dc.identifier.citationL. Trache, A. Azhari, H. L. Clark, Carl A. Gagliardi, Y. W. Lui, A. M. Mukhamedzhanov, Robert E. Tribble and F. Carstoiu. Phys.Rev.C 58 2715-2719 1998. "Copyright (1998) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.58.2715
dc.identifier.urihttps://hdl.handle.net/1969.1/126878
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractThe C-13(N-14,C-13)N-14 proton exchange reaction has been measured at an incident energy of 162 MeV. Angular distributions were obtained for proton transfer to the ground and low-lying excited states in N-14. Elastic scattering of N-14 On C-13 also was measured out to the rainbow angle region in order to find reliable optical model potentials. Asymptotic normalization coefficients for the system C-13+p --> N-14 have been found for the ground state and the excited states at 2.313, 3.948, 5.106, and 5.834 MeV in N-14. These asymptotic normalization coefficients will be used in a determination of the S factor for Be-7(p, gamma)B-8 at solar energies from a measurement of the proton transfer reaction N-14(Be-7,B-8)C-13. [S0556-2813(98)03111-2].en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectASTROPHYSICAL S-FACTORen
dc.subjectSCATTERINGen
dc.subjectPhysicsen
dc.titleAsymptotic normalization coefficients for C-13+p -> N-14en
dc.typeArticleen
local.departmentPhysics and Astronomyen


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