Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions

Detalhes bibliográficos
Autor(a) principal: Aguiar, Carlos Eduardo
Data de Publicação: 2004
Outros Autores: Andrade, Rone Peterson Galvão de, Grassi, Frederique Marie-Brigitte Sylvie, Hama, Yogiro, Socolowski Junior, Otavio
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da FURG (RI FURG)
Texto Completo: http://repositorio.furg.br/handle/1/3399
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.
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spelling Aguiar, Carlos EduardoAndrade, Rone Peterson Galvão deGrassi, Frederique Marie-Brigitte SylvieHama, YogiroSocolowski Junior, Otavio2013-05-21T19:08:08Z2013-05-21T19:08:08Z2004AGUIAR, Carlos Eduardo et al. Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions. Brazilian Journal of Physics, v. 34, n. 1, p. 319-321, 2004. Disponível em: <http://www.scielo.br/scielo.php?pid=S0103-97332004000200040&script=sci_arttext>. Acesso em: 26 abr. 2013.0103-9733http://repositorio.furg.br/handle/1/3399doi.org/10.1590/S0103-97332004000200040Using 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.engComparison between classification using impact parameter and using number of participants in relativistic nuclear collisionsinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleinfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da FURG (RI FURG)instname:Universidade Federal do Rio Grande (FURG)instacron:FURGORIGINALComparison Between Classification Using Impact Parameter and Using Number of Participants in Relativistic Nuclear Collisions..pdfComparison Between Classification Using Impact Parameter and Using Number of Participants in Relativistic Nuclear Collisions..pdfapplication/pdf331687https://repositorio.furg.br/bitstream/1/3399/1/Comparison%20Between%20Classification%20Using%20Impact%20Parameter%20and%20Using%20Number%20of%20Participants%20in%20Relativistic%20Nuclear%20Collisions..pdff76b1d2c09f0ca05adbdebe0889bc40bMD51open accessLICENSElicense.txtlicense.txttext/plain; charset=utf-81724https://repositorio.furg.br/bitstream/1/3399/2/license.txt5b92b9704b4f13242d70e45ddef35a68MD52open access1/33992013-05-21 16:08:08.611open accessoai:repositorio.furg.br:1/3399w4kgbmVjZXNzw6FyaW8gY29uY29yZGFyIGNvbSBhIGxpY2Vuw6dhIGRlIGRpc3RyaWJ1acOnw6NvIG7Do28tZXhjbHVzaXZhLAphbnRlcyBxdWUgbyBkb2N1bWVudG8gcG9zc2EgYXBhcmVjZXIgbm8gUmVwb3NpdMOzcmlvLiBQb3IgZmF2b3IsIGxlaWEgYQpsaWNlbsOnYSBhdGVudGFtZW50ZS4gQ2FzbyBuZWNlc3NpdGUgZGUgYWxndW0gZXNjbGFyZWNpbWVudG8gZW50cmUgZW0KY29udGF0byBhdHJhdsOpcyBkZTogcmVwb3NpdG9yaW9AZnVyZy5iciBvdSAweHggNTMgMzIzMy02NzA2LgoKTElDRU7Dh0EgREUgRElTVFJJQlVJw4fDg08gTsODTy1FWENMVVNJVkEKCkFvIGFzc2luYXIgZSBlbnRyZWdhciBlc3RhIGxpY2Vuw6dhLCBvL2EgU3IuL1NyYS4gKGF1dG9yIG91IGRldGVudG9yIGRvcyBkaXJlaXRvcyBkZSBhdXRvcik6CgphKSBDb25jZWRlIMOgIFVuaXZlcnNpZGFkZSBGZWRlcmFsIGRlIFJpbyBHcmFuZGUgLSAgRlVSRyBvIGRpcmVpdG8gbsOjby1leGNsdXNpdm8gZGUgcmVwcm9kdXppciwgY29udmVydGVyIChjb21vIGRlZmluaWRvIGFiYWl4byksIGNvbXVuaWNhciBlL291IGRpc3RyaWJ1aXIgbyBkb2N1bWVudG8gZW50cmVndWUgKGluY2x1aW5kbyBvIHJlc3Vtby9hYnN0cmFjdCkgZW0KZm9ybWF0byBkaWdpdGFsIG91IGltcHJlc3NvIGUgZW0gcXVhbHF1ZXIgbWVpby4KCmIpIERlY2xhcmEgcXVlIG8gZG9jdW1lbnRvIGVudHJlZ3VlIMOpIHNldSB0cmFiYWxobyBvcmlnaW5hbCwgZSBxdWUKZGV0w6ltIG8gZGlyZWl0byBkZSBjb25jZWRlciBvcyBkaXJlaXRvcyBjb250aWRvcyBuZXN0YSBsaWNlbsOnYS4gRGVjbGFyYSB0YW1iw6ltIHF1ZSBhIGVudHJlZ2EgZG8gZG9jdW1lbnRvIG7Do28gaW5mcmluZ2UsIHRhbnRvIHF1YW50byBsaGUgw6kgcG9zc8OtdmVsIHNhYmVyLCBvcyBkaXJlaXRvcyBkZSBxdWFscXVlciBvdXRyYSBwZXNzb2Egb3UgZW50aWRhZGUuCgpjKSBTZSBvIGRvY3VtZW50byBlbnRyZWd1ZSBjb250w6ltIG1hdGVyaWFsIGRvIHF1YWwgbsOjbyBkZXTDqW0gb3MKZGlyZWl0b3MgZGUgYXV0b3IsIGRlY2xhcmEgcXVlIG9idGV2ZSBhdXRvcml6YcOnw6NvIGRvIGRldGVudG9yIGRvcwpkaXJlaXRvcyBkZSBhdXRvciBwYXJhIGNvbmNlZGVyIMOgIEZVUkcgb3MgZGlyZWl0b3MgcmVxdWVyaWRvcyBwb3IgZXN0YSBsaWNlbsOnYSwgZSBxdWUgZXNzZSBtYXRlcmlhbCBjdWpvcyBkaXJlaXRvcyBzw6NvIGRlIHRlcmNlaXJvcyBlc3TDoSBjbGFyYW1lbnRlIGlkZW50aWZpY2FkbyBlIHJlY29uaGVjaWRvIG5vIHRleHRvIG91IGNvbnRlw7pkbyBkbyBkb2N1bWVudG8gZW50cmVndWUuCgpTZSBvIGRvY3VtZW50byBlbnRyZWd1ZSDDqSBiYXNlYWRvIGVtIHRyYWJhbGhvIGZpbmFuY2lhZG8gb3UgYXBvaWFkbwpwb3Igb3V0cmEgaW5zdGl0dWnDp8OjbyBxdWUgbsOjbyBhIEZVUkcsIGRlY2xhcmEgcXVlIGN1bXByaXUgcXVhaXNxdWVyIG9icmlnYcOnw7VlcyBleGlnaWRhcyBwZWxvIHJlc3BlY3Rpdm8gY29udHJhdG8gb3UgYWNvcmRvLgoKQSBGVVJHIGlkZW50aWZpY2Fyw6EgY2xhcmFtZW50ZSBvKHMpIHNldSAocykgbm9tZSAocykgY29tbyBvIChzKSBhdXRvciAoZXMpIG91IGRldGVudG9yIChlcykgZG9zIGRpcmVpdG9zIGRvIGRvY3VtZW50byBlbnRyZWd1ZSwgZSBuw6NvIGZhcsOhIHF1YWxxdWVyIGFsdGVyYcOnw6NvLCBwYXJhIGFsw6ltIGRhcyBwZXJtaXRpZGFzIHBvciBlc3RhIGxpY2Vuw6dhLgo=Repositório InstitucionalPUBhttps://repositorio.furg.br/oai/request || http://200.19.254.174/oai/requestopendoar:2013-05-21T19:08:08Repositório Institucional da FURG (RI FURG) - Universidade Federal do Rio Grande (FURG)false
dc.title.pt_BR.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, Carlos Eduardo
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, Carlos Eduardo
author_facet Aguiar, Carlos Eduardo
Andrade, Rone Peterson Galvão de
Grassi, Frederique Marie-Brigitte Sylvie
Hama, Yogiro
Socolowski Junior, Otavio
author_role author
author2 Andrade, Rone Peterson Galvão de
Grassi, Frederique Marie-Brigitte Sylvie
Hama, Yogiro
Socolowski Junior, Otavio
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Aguiar, Carlos Eduardo
Andrade, Rone Peterson Galvão de
Grassi, Frederique Marie-Brigitte Sylvie
Hama, Yogiro
Socolowski Junior, Otavio
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.issued.fl_str_mv 2004
dc.date.accessioned.fl_str_mv 2013-05-21T19:08:08Z
dc.date.available.fl_str_mv 2013-05-21T19:08:08Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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status_str publishedVersion
dc.identifier.citation.fl_str_mv AGUIAR, Carlos Eduardo et al. Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions. Brazilian Journal of Physics, v. 34, n. 1, p. 319-321, 2004. Disponível em: <http://www.scielo.br/scielo.php?pid=S0103-97332004000200040&script=sci_arttext>. Acesso em: 26 abr. 2013.
dc.identifier.uri.fl_str_mv http://repositorio.furg.br/handle/1/3399
dc.identifier.issn.none.fl_str_mv 0103-9733
dc.identifier.doi.pt_BR.fl_str_mv doi.org/10.1590/S0103-97332004000200040
identifier_str_mv AGUIAR, Carlos Eduardo et al. Comparison between classification using impact parameter and using number of participants in relativistic nuclear collisions. Brazilian Journal of Physics, v. 34, n. 1, p. 319-321, 2004. Disponível em: <http://www.scielo.br/scielo.php?pid=S0103-97332004000200040&script=sci_arttext>. Acesso em: 26 abr. 2013.
0103-9733
doi.org/10.1590/S0103-97332004000200040
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