dc.contributor | Universidade Estadual Paulista (UNESP) | |
dc.contributor | Universidade de São Paulo (USP) | |
dc.contributor | Universidade Federal de Alfenas | |
dc.contributor | Universidade Federal do Rio de Janeiro (UFRJ) | |
dc.date.accessioned | 2022-04-28T19:06:22Z | |
dc.date.accessioned | 2022-12-20T01:04:28Z | |
dc.date.available | 2022-04-28T19:06:22Z | |
dc.date.available | 2022-12-20T01:04:28Z | |
dc.date.created | 2022-04-28T19:06:22Z | |
dc.date.issued | 2017-06-15 | |
dc.identifier | Physical Review C, v. 95, n. 6, 2017. | |
dc.identifier | 2469-9993 | |
dc.identifier | 2469-9985 | |
dc.identifier | http://hdl.handle.net/11449/220866 | |
dc.identifier | 10.1103/PhysRevC.95.064908 | |
dc.identifier | 2-s2.0-85020836172 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/5400995 | |
dc.description.abstract | Measurements of di-hadron azimuthal correlations at different centralities for Au+Au collisions at 200A GeV were reported by the PHENIX Collaboration. The data were presented for different ranges of transverse momentum. In particular, it was observed that the away-side correlation evolves from a double- to a single-peak structure when the centrality decreases. In this work, we show that these features naturally appear due to an interplay between the centrality-dependent smooth background elliptic flow and the one produced by event-by-event fluctuating peripheral tubes. To compare with the PHENIX data, we also carry out numerical simulations by using a hydrodynamical code nexspherio, and calculate the correlations by both cumulant and the ZYAM method employed by the PHENIX Collaboration. Our results are in reasonable agreement with the data. A brief discussion on the physical content of the present model and its difference from other viewpoints is also presented. | |
dc.language | eng | |
dc.relation | Physical Review C | |
dc.source | Scopus | |
dc.title | Hydrodynamic approach to the centrality dependence of di-hadron correlations | |
dc.type | Artículos de revistas | |