Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions
Autor(a) principal: | |
---|---|
Data de Publicação: | 2004 |
Outros Autores: | , , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Brazilian Journal of Physics |
Texto Completo: | http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000200040 |
Resumo: | 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. |
id |
SBF-2_c316fd04aafb4914c9a64171a2076e42 |
---|---|
oai_identifier_str |
oai:scielo:S0103-97332004000200040 |
network_acronym_str |
SBF-2 |
network_name_str |
Brazilian Journal of Physics |
repository_id_str |
|
spelling |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisionsUsing 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.Sociedade Brasileira de Física2004-03-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000200040Brazilian Journal of Physics v.34 n.1a 2004reponame:Brazilian Journal of Physicsinstname:Sociedade Brasileira de Física (SBF)instacron:SBF10.1590/S0103-97332004000200040info:eu-repo/semantics/openAccessAguiar,C.E.Andrade,R.Grassi,F.Hama,Y.Kodama,T.Osada,T.Socolowski Jr.,O.eng2004-05-11T00:00:00Zoai:scielo:S0103-97332004000200040Revistahttp://www.sbfisica.org.br/v1/home/index.php/pt/ONGhttps://old.scielo.br/oai/scielo-oai.phpsbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br1678-44480103-9733opendoar:2004-05-11T00:00Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)false |
dc.title.none.fl_str_mv |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
title |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
spellingShingle |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions Aguiar,C.E. |
title_short |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
title_full |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
title_fullStr |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
title_full_unstemmed |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
title_sort |
Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions |
author |
Aguiar,C.E. |
author_facet |
Aguiar,C.E. Andrade,R. Grassi,F. Hama,Y. Kodama,T. Osada,T. Socolowski Jr.,O. |
author_role |
author |
author2 |
Andrade,R. Grassi,F. Hama,Y. Kodama,T. Osada,T. Socolowski Jr.,O. |
author2_role |
author author author author author author |
dc.contributor.author.fl_str_mv |
Aguiar,C.E. Andrade,R. Grassi,F. Hama,Y. Kodama,T. Osada,T. Socolowski Jr.,O. |
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. |
publishDate |
2004 |
dc.date.none.fl_str_mv |
2004-03-01 |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000200040 |
url |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000200040 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
10.1590/S0103-97332004000200040 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
text/html |
dc.publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
dc.source.none.fl_str_mv |
Brazilian Journal of Physics v.34 n.1a 2004 reponame:Brazilian Journal of Physics instname:Sociedade Brasileira de Física (SBF) instacron:SBF |
instname_str |
Sociedade Brasileira de Física (SBF) |
instacron_str |
SBF |
institution |
SBF |
reponame_str |
Brazilian Journal of Physics |
collection |
Brazilian Journal of Physics |
repository.name.fl_str_mv |
Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF) |
repository.mail.fl_str_mv |
sbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br |
_version_ |
1754734860764708865 |