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Publicação:
Possible origin of RHIC Rout/Rsid HBT results

dc.contributor.authorPadula, Sandra S. [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionMS106
dc.contributor.institutionBrookhaven National Laboratory
dc.date.accessioned2014-05-27T11:20:38Z
dc.date.available2014-05-27T11:20:38Z
dc.date.issued2003-03-10
dc.description.abstractThe effects of opacity of the nuclei together with a blackbody type of emission along the system history are considered as a means to explain the ratio Rout/Rsid observed by STAR and PHENIX collaborations at RHIC. Within our model, no flow is required to explain the data trend of this ratio for large surface emissivities. © 2003 Elsevier Science B.V. All rights reserved.en
dc.description.affiliationInstitute de Física Teórica Universidade Estadual Paulista, São Paulo - SP
dc.description.affiliationTheoretical Physics FERMILAB MS106, P.O. Box 500, Batavia, IL 60510
dc.description.affiliationNuclear Theory Group Brookhaven National Laboratory, Upton, NY 11973
dc.description.affiliationUnespInstitute de Física Teórica Universidade Estadual Paulista, São Paulo - SP
dc.identifierhttp://dx.doi.org/10.1016/S0375-9474(02)01550-6
dc.identifier.citationNuclear Physics A, v. 715, p. 637C-640C, 2003.
dc.identifier.doi10.1016/S0375-9474(02)01550-6
dc.identifier.issn0375-9474
dc.identifier.scopus2-s2.0-17544372927
dc.identifier.urihttp://hdl.handle.net/11449/67230
dc.identifier.wosWOS:000181737500090
dc.language.isoeng
dc.relation.ispartofNuclear Physics A
dc.relation.ispartofjcr1.992
dc.relation.ispartofsjr0,938
dc.rights.accessRightsAcesso aberto
dc.sourceScopus
dc.titlePossible origin of RHIC Rout/Rsid HBT resultsen
dc.typeTrabalho apresentado em evento
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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