Energy And System-size Dependence Of Two- And Four-particle V 2 Measurements In Heavy-ion Collisions At √s Nn=62.4 And 200 Gev And Their Implications On Flow Fluctuations And Nonflow

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dc.date2012
dc.date2015-06-26T20:29:57Z
dc.date2015-11-26T14:26:31Z
dc.date2015-06-26T20:29:57Z
dc.date2015-11-26T14:26:31Z
dc.date.accessioned2018-03-28T21:29:35Z
dc.date.available2018-03-28T21:29:35Z
dc.identifier
dc.identifierPhysical Review C - Nuclear Physics. , v. 86, n. 1, p. - , 2012.
dc.identifier5562813
dc.identifier10.1103/PhysRevC.86.014904
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-84864416587&partnerID=40&md5=114adf2b00c09ddb72a90a41ded1a75f
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/97187
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/97187
dc.identifier2-s2.0-84864416587
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1246102
dc.descriptionWe present STAR measurements of azimuthal anisotropy by means of the two- and four-particle cumulants v 2 (v 2{2} and v 2{4}) for Au+Au and Cu+Cu collisions at center-of-mass energies √sN N=62.4 and 200 GeV. The difference between v 2 {2 }2 and v 2 {4 }2 is related to v 2 fluctuations (σv 2) and nonflow (δ 2). We present an upper limit to σv 2/v 2. Following the assumption that eccentricity fluctuations σ dominate v 2 fluctuations σv 2v 2≈σ we deduce the nonflow implied for several models of eccentricity fluctuations that would be required for consistency with v 2{2} and v 2{4}. We also present results on the ratio of v 2 to eccentricity. © 2012 American Physical Society.
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dc.languageen
dc.publisher
dc.relationPhysical Review C - Nuclear Physics
dc.rightsaberto
dc.sourceScopus
dc.titleEnergy And System-size Dependence Of Two- And Four-particle V 2 Measurements In Heavy-ion Collisions At √s Nn=62.4 And 200 Gev And Their Implications On Flow Fluctuations And Nonflow
dc.typeArtículos de revistas


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