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DOI 10.1103/PhysRevLett.73.3070
Title Fragmentation of necklike structures
Creator/Author Montoya, C.P. ; Lynch, W.G. ; Bowman, D.R. ; Peaslee, G.F. ; Carlin, N. ; de Souza, R.T. ; Gelbke, C.K. ; Gong, W.G. ; Kim, Y.D. ; Lisa, M.A. ; Phair, L. ; Tsang, M.B. ; Webster, J.B. ; Williams, C. (National Superconducting Cyclotron Laboratory and Department of Physics Astronomy, Michigan State University, East Lansing, Michigan 48824 (United States)) ; Colonna, N. ; Hanold, K. ; McMahan, M.A. ; Wozniak, G.J. ; Moretto, L.G. (Nuclear Science Division and Accelerator and Fusion Research Division, Lawrence Berkeley Laboratory, Berkeley, California 94720 (United States))
Publication Date1994 Dec 05
OSTI IdentifierOSTI ID: 6703800
DOE Contract NumberAC03-76SF00098
Other Number(s)Journal ID: ISSN 0031-9007; CODEN: PRLTAO
Resource TypeJournal Article
Resource RelationJournal: Physical Review Letters; (United States); Journal Volume: 73:23
Subject73 NUCLEAR PHYSICS AND RADIATION PHYSICS; COPPER; XENON 129 REACTIONS; NUCLEAR FRAGMENTS; EMISSION; CHARGE DISTRIBUTION; CYLINDRICAL CONFIGURATION; EVAPORATION; FRAGMENTATION; HEAVY ION REACTIONS; CHARGED-PARTICLE REACTIONS; CONFIGURATION; ELEMENTS; METALS; NUCLEAR REACTIONS; PHASE TRANSFORMATIONS; TRANSITION ELEMENTS
Description/Abstract Intermediate mass fragment (IMF: 3[le][ital Z][le]20) emission from necklike structures joining projectilelike and targetlike residues has been observed for peripheral [sup 129]Xe+[sup nat]Cu collisions at [ital E]/[ital A]=50 MeV. These fragments are emitted primarily at velocities between those of the projectilelike and targetlike residues. Relative to the charge distribution of fragments evaporated from projectilelike residues, the distribution for neck'' emission shows an enhanced emission for fragments with 4[le][ital Z][sub IMF][le]12. This feature is consistent with expectations for the fragmentation of a noncompact cylindrical configuration.
Country of PublicationUnited States
LanguageEnglish
FormatSize: Pages: 3070-3073
System Entry Date2008 Aug 18

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