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dc.creatorAzhari, A.
dc.creatorBurjan, V.
dc.creatorCarstoiu, F.
dc.creatorGagliardi, Carl A.
dc.creatorKroha, V.
dc.creatorMukhamedzhanov, AM
dc.creatorTang, X.
dc.creatorTrache, L.
dc.creatorTribble, Robert E.
dc.date.accessioned2011-09-13T21:27:52Z
dc.date.available2011-09-13T21:27:52Z
dc.date.issued1999
dc.identifier.citationA. Azhari, V. Burjan, F. Carstoiu, Carl A. Gagliardi, V. Kroha, A. M. Mukhamedzhanov, X. Tang, L. Trache and Robert E. Tribble. Phys.Rev.C 60 055803 1999. "Copyright (1999) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.60.055803
dc.identifier.urihttps://hdl.handle.net/1969.1/126892
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractThe N-14(Be-7,B-8)C-13 reaction was studied using an 85 MeV Be-7 radioactive beam. The asymptotic normalization coefficients for the virtual transitions Be-7+pB-8 were determined from the measured cross section. These coefficients specify the amplitude of the tail of the B-8 overlap function in the Be-7+ p channel, and were used to calculate the astrophysical S factor for the direct capture reaction Be-7(p,gamma)B-8 at solar energies S-17(0). We find that S-17(0) = 16.6 +/- 1.9 eV b. [S0556-2813(99)01111-5].en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectASYMPTOTIC NORMALIZATION COEFFICIENTSen
dc.subjectCROSS-SECTIONen
dc.subjectLOW ENERGIESen
dc.subjectBE-7(D,N)B-8 REACTIONen
dc.subjectCOULOMB DISSOCIATIONen
dc.subjectANGULAR-DISTRIBUTIONen
dc.subjectS-17(0) FACTORen
dc.subjectNUCLEIen
dc.subjectMODELen
dc.subjectB-8en
dc.subjectPhysicsen
dc.titleThe N-14(Be-7,B-8)C-13 reaction and the Be-7(p,gamma)B-8 S factoren
dc.typeArticleen
local.departmentPhysics and Astronomyen


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