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Origin of the Structures in the C-12(o-16,alpha) Reaction - Dominance of Ne-20-Star and O-16-Star Sequential Alpha-Decay Processes

dc.creatorMurakami, T.
dc.creatorUngricht, E.
dc.creatorTakahashi, N.
dc.creatorLui, YW
dc.creatorMihara, Y.
dc.creatorNeese, R. E.
dc.creatorTakada, E.
dc.creatorTanner, D. M.
dc.creatorTribble, Robert E.
dc.creatorNagatani, K.
dc.date.accessioned2011-09-13T21:26:12Z
dc.date.available2011-09-13T21:26:12Z
dc.date.issued1984
dc.identifier.citationT. Murakami, E. Ungricht, N. Takahashi, Y. W. Lui, Y. Mihara, R. E. Neese, E. Takada, D. M. Tanner, Robert E. Tribble and K. Nagatani. Phys.Rev.C 29 847-860 1984. "Copyright (1984) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.29.847
dc.identifier.urihttps://hdl.handle.net/1969.1/126775
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectPhysicsen
dc.titleOrigin of the Structures in the C-12(o-16,alpha) Reaction - Dominance of Ne-20-Star and O-16-Star Sequential Alpha-Decay Processesen
dc.typeArticleen
local.departmentPhysics and Astronomyen


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