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dc.creatorBem, P.
dc.creatorBurjan, V.
dc.creatorKroha, V.
dc.creatorNovak, J.
dc.creatorPiskor, S.
dc.creatorSimeckova, E.
dc.creatorVincour, J.
dc.creatorGagliardi, Carl A.
dc.creatorMukhamedzhanov, AM
dc.creatorTribble, Robert E.
dc.date.accessioned2011-09-13T21:25:35Z
dc.date.available2011-09-13T21:25:35Z
dc.date.issued2000
dc.identifier.citationP. Bem, V. Burjan, V. Kroha, J. Novak, S. Piskor, E. Simeckova, J. Vincour, Carl A. Gagliardi, A. M. Mukhamedzhanov and Robert E. Tribble. Phys.Rev.C 62 024320 2000. "Copyright (2000) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.113/PhysRevC.62.024320
dc.identifier.urihttps://hdl.handle.net/1969.1/126899
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractThe C-13(He-3,d) N-14 proton transfer reaction has been measured at an incident energy of 26.3 MeV. Angular distributions for proton transfer to the ground state and excited states at 2.313 and 3.948 MeV in N-14 are analyzed within the framework of the modified DWBA. Asymptotic normalization coefficients (ANC's) defining the amplitude of the tails of the N-14 bound-state wave functions in the C-13+p channel are extracted that are in excellent agreement with values found previously with the C-13(N-14,C-13)N-14 reaction. We conclude that C-p1/2(2)=18.2(9) fm(-1) and C-p3/2(2) = 0.91(14) fm(-1) for the virtual decay N-14(g.s.) --> C-13+p. These are necessary for the analysis of the N-14(Be-7, B-8)C-13 and N-14( C-11, N-12) C-13 reactions to extract the ANC's far Be-7+p --> B-8 and C-11+p-->N-12, which determine the direct radiative capture cross sections Be-7(p,gamma)B-8 and C-11(p,gamma)N-12 at astrophysical energies.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectBE-7(P,GAMMA)B-8 S-FACTORen
dc.subjectPhysicsen
dc.titleAsymptotic normalization coefficients for N-14 C-13+p from C-13(He-3,d)N-14en
dc.typeArticleen
local.departmentPhysics and Astronomyen


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