| dc.creator |
Aguiar C.E. |
|
| dc.creator |
Andrade R. |
|
| dc.creator |
Grassi F. |
|
| dc.creator |
Hama Y. |
|
| dc.creator |
Kodama T. |
|
| dc.creator |
Osada T. |
|
| dc.creator |
Socolowski Jr. O. |
|
| dc.date |
2004 |
|
| dc.date.accessioned |
2013-06-01T11:34:18Z |
|
| dc.date.available |
2013-06-01T11:34:18Z |
|
| dc.date.issued |
2013-06-01 |
|
| dc.identifier |
http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000200040 |
|
| dc.identifier |
http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2004&volume=34&issue=1a&spage=319 |
|
| dc.identifier.uri |
http://koha.mediu.edu.my:8181/jspui/handle/123456789/8582 |
|
| dc.description |
Using 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.publisher |
Sociedade Brasileira de Física |
|
| dc.source |
Brazilian Journal of Physics |
|
| dc.title |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
|