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dc.creatorLin, ZW
dc.creatorKo, Che Ming
dc.creatorLi, Ba
dc.creatorZhang, B.
dc.creatorPal, S.
dc.date.accessioned2011-09-13T21:25:31Z
dc.date.available2011-09-13T21:25:31Z
dc.date.issued2005
dc.identifier.citationZ. W. Lin, Che Ming Ko, Ba Li, B. Zhang and S. Pal. Phys.Rev.C 72 064901 2005. "Copyright (2005) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.72.064901
dc.identifier.urihttps://hdl.handle.net/1969.1/127001
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractWe describe in detail how the different components of a multiphase transport (AMPT) model that uses the heavy ion jet interaction generator (HIJING) for generating the initial conditions, Zhang's parton cascade (ZPC) for modeling partonic scatterings, the Lund string fragmentation model or a quark coalescence model for hadronization, and a relativistic transport (ART) model for treating hadronic scatterings are improved and combined to give a coherent description of the dynamics of relativistic heavy ion collisions. We also explain the way parameters in the model are determined and discuss the sensitivity of predicted results to physical input in the model. Comparisons of these results to experimental data, mainly from heavy ion collisions at the BNL Relativistic Heavy Ion Collider, are then made in order to extract information on the properties of the hot dense matter formed in these collisions.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectQUARK-GLUON PLASMAen
dc.subjectULTRARELATIVISTIC NUCLEAR COLLISIONSen
dc.subjectPHI-MESONen
dc.subjectPRODUCTIONen
dc.subjectPLUS AU COLLISIONSen
dc.subjectANTIPROTON-PROTON COLLISIONSen
dc.subjectQUANTUMen
dc.subjectMOLECULAR-DYNAMICSen
dc.subjectSUPERDENSE HADRONIC MATTERen
dc.subjectLOW-MASS DILEPTONSen
dc.subjectHIGH-DENSITY QCDen
dc.subjectELLIPTIC FLOWen
dc.subjectPhysicsen
dc.titleMultiphase transport model for relativistic heavy ion collisionsen
dc.typeArticleen
local.departmentPhysics and Astronomyen


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