Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8582
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dc.creatorAguiar C.E.-
dc.creatorAndrade R.-
dc.creatorGrassi F.-
dc.creatorHama Y.-
dc.creatorKodama T.-
dc.creatorOsada T.-
dc.creatorSocolowski Jr. O.-
dc.date2004-
dc.date.accessioned2013-06-01T11:34:18Z-
dc.date.available2013-06-01T11:34:18Z-
dc.date.issued2013-06-01-
dc.identifierhttp://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000200040-
dc.identifierhttp://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2004&volume=34&issue=1a&spage=319-
dc.identifier.urihttp://koha.mediu.edu.my:8181/jspui/handle/123456789/8582-
dc.descriptionUsing the hydrodynamical code NeXSPheRIO, we compare predictions as usually done in hydrodynamics, using centrality windows defined through the impact parameter, and as obtainable experimentally, using windows in participant number.-
dc.publisherSociedade Brasileira de Física-
dc.sourceBrazilian Journal of Physics-
dc.titleComparison between classification using impact parameter and using number of participants in relativistic nuclear collisions-
Appears in Collections:Physics and Astronomy

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