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dc.creatorCarstoiu, F.
dc.creatorTrache, L.
dc.creatorGagliardi, Carl A.
dc.creatorTribble, Robert E.
dc.creatorMukhamedzhanov, AM.
dc.date.accessioned2011-09-13T21:27:19Z
dc.date.available2011-09-13T21:27:19Z
dc.date.issued2001
dc.identifier.citationF. Carstoiu, L. Trache, Carl A. Gagliardi, Robert E. Tribble and A. M. Mukhamedzhanov. Phys.Rev.C 63 054310 2001. "Copyright (2001) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.63.054310
dc.identifier.urihttps://hdl.handle.net/1969.1/126905
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractThe experimental asymptotic normalization coefficient determined from peripheral transfer reactions is used to obtain the root-mean-square radius of the wave function for the loosely bound proton in SB. It is shown that the asymptotic region contributes most and that matching of the interior wave function with the asymptotic part yields a nearly model-independent radius. We obtain [r(2)] (1/2) = 4.20 +/- 0.22 fm for the root-mean-square (rms) radius of the last proton, much larger than the rms radius of the Be-7 core. This large value and the fact that the asymptotic part of the proton wave function contributes 85% to the rms radius are good sign that B-8 is a halo nucleus.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectCROSS-SECTION MEASUREMENTSen
dc.subjectBE-7(P,GAMMA)B-8 S-FACTORen
dc.subjectPROTON-HALOen
dc.subjectCOULOMB DISSOCIATIONen
dc.subjectNUCLEIen
dc.subjectBREAKUPen
dc.subjectMODELen
dc.subjectMEV/NUCLEONen
dc.subjectLI-8en
dc.subjectDENSITIESen
dc.subjectPhysicsen
dc.titleRadius of B-8 halo from the asymptotic normalization coefficienten
dc.typeArticleen
local.departmentPhysics and Astronomyen


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