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dc.creatorLi, Zeng-Hua
dc.creatorChen, Lie-Wen
dc.creatorKo, Che Ming
dc.creatorLi, Bao-An
dc.creatorMa, Hong-Ru.
dc.date.accessioned2011-09-13T21:26:13Z
dc.date.available2011-09-13T21:26:13Z
dc.date.issued2006
dc.identifier.citationZeng-Hua Li, Lie-Wen Chen, Che Ming Ko, Bao-An Li and Hong-Ru Ma. Phys.Rev.C 74 044613 2006. "Copyright (2006) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.74.044613
dc.identifier.urihttps://hdl.handle.net/1969.1/127020
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractUsing the relativistic impulse approximation with the Love-Franey NN scattering amplitude developed by Murdock and Horowitz, we investigate the low-energy (100 <= E(kin)<= 400 MeV) behavior of the nucleon Dirac optical potential, the Schrodinger-equivalent potential, and the nuclear symmetry potential in isospin asymmetric nuclear matter. We find that the nuclear symmetry potential at fixed baryon density decreases with increasing nucleon energy. In particular, the nuclear symmetry potential at saturation density changes from positive to negative values at nucleon kinetic energy of about 200 MeV. Furthermore, the obtained energy and density dependence of the nuclear symmetry potential is consistent with those of the isospin- and momentum-dependent MDI interaction with x=0, which has been found to describe reasonably well both the isospin diffusion data from heavy-ion collisions and the empirical neutron-skin thickness of (208)Pb.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectHEAVY-ION COLLISIONSen
dc.subjectPOINT-COUPLING MODELSen
dc.subjectNEUTRON-RICH NUCLEIen
dc.subjectMEAN-FIELD THEORYen
dc.subjectELASTIC-SCATTERINGen
dc.subjectDIRAC-EQUATIONen
dc.subjectINTERMEDIATEen
dc.subjectENERGIESen
dc.subjectEFFECTIVE-MASSen
dc.subjectFINITE NUCLEIen
dc.subjectDENSITYen
dc.subjectPhysicsen
dc.titleNuclear symmetry potential in the relativistic impulse approximation RID A-2398-2009 RID C-6879-2009en
dc.typeArticleen
local.departmentPhysics and Astronomyen


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