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dc.creatorAzhari, A.en_US
dc.creatorBurjan, V.en_US
dc.creatorCarstoiu, F.en_US
dc.creatorGagliardi, Carl A.en_US
dc.creatorKroha, V.en_US
dc.creatorMukhamedzhanov, AMen_US
dc.creatorTang, X.en_US
dc.creatorTrache, L.en_US
dc.creatorTribble, Robert E.en_US
dc.date.accessioned2011-09-13T21:27:52Z
dc.date.available2011-09-13T21:27:52Z
dc.date.issued1999en_US
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_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.60.055803en_US
dc.identifier.urihttp://hdl.handle.net/1969.1/126892
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en_US
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_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectASYMPTOTIC NORMALIZATION COEFFICIENTSen_US
dc.subjectCROSS-SECTIONen_US
dc.subjectLOW ENERGIESen_US
dc.subjectBE-7(D,N)B-8 REACTIONen_US
dc.subjectCOULOMB DISSOCIATIONen_US
dc.subjectANGULAR-DISTRIBUTIONen_US
dc.subjectS-17(0) FACTORen_US
dc.subjectNUCLEIen_US
dc.subjectMODELen_US
dc.subjectB-8en_US
dc.subjectPhysicsen_US
dc.titleThe N-14(Be-7,B-8)C-13 reaction and the Be-7(p,gamma)B-8 S factoren_US
dc.typeArticleen_US
local.departmentPhysics and Astronomyen_US


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