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dc.creatorChen, LW
dc.creatorKo, Che Ming
dc.creatorLi, Ba.
dc.date.accessioned2011-09-13T21:27:49Z
dc.date.available2011-09-13T21:27:49Z
dc.date.issued2003
dc.identifier.citationLW Chen, Che Ming Ko and BA Li. Phys.Rev.C 68 017601 2003. "Copyright (2003) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.68.017601
dc.identifier.urihttp://hdl.handle.net/1969.1/126938
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractUsing an isospin-dependent transport model for heavy-ion collisions induced by neutron-rich nuclei at intermediate energies, we study the production of light clusters such as deuteron, triton, and He-3 via coalescence of nucleons. We find that both the yields and the energy spectra of these light clusters are affected significantly by the density dependence of nuclear symmetry energy, with a stiffer symmetry energy giving a larger yield.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectHEAVY-ION COLLISIONSen
dc.subjectNEUTRON-STAR STRUCTUREen
dc.subjectISOSPIN-DEPENDENCEen
dc.subjectMICROSCOPIC CALCULATIONen
dc.subjectINTERMEDIATE ENERGIESen
dc.subjectDIFFERENTIAL FLOWen
dc.subjectCOLLECTIVE FLOWen
dc.subjectCROSS-SECTIONSen
dc.subjectEQUATIONen
dc.subjectMATTERen
dc.subjectPhysicsen
dc.titleLight clusters production as a probe to nuclear symmetry energy RID A-2398-2009en
dc.typeArticleen
local.departmentPhysics and Astronomyen


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