Please use this identifier to cite or link to this item: http://idr.niser.ac.in:8080/jspui/handle/123456789/1096
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dc.contributor.authorMohanty, Bedangadas-
dc.date.accessioned2024-12-04T07:47:47Z-
dc.date.available2024-12-04T07:47:47Z-
dc.date.issued2013-07-15-
dc.identifier.citationAdamczyk, L., Adkins, J. K., Agakishiev, G., Aggarwal, M. M., Ahammed, Z., Alakhverdyants, A. V., … Zyzak, M. (2013). Third harmonic flow of charged particles in Au+Au collisions atsNN=200 GeV. Physical Review C: Nuclear Physics, 88(1).en_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevC.88.014904-
dc.identifier.urihttp://idr.niser.ac.in:8080/jspui/handle/123456789/1096-
dc.description.abstractWe report measurements of the third harmonic coefficient of the azimuthal anisotropy, v3, known as triangular flow. The analysis is for charged particles in Au+Au collisions at √sNN=200 GeV, based on data from the STAR experiment at the BNL Relativistic Heavy Ion Collider. Two-particle correlations as a function of their pseudorapidity separation are fit with narrow and wide Gaussians. Measurements of triangular flow are extracted from the wide Gaussian, from two-particle cumulants with a pseudorapidity gap, and also from event plane analysis methods with a large pseudorapidity gap between the particles and the event plane. These results are reported as a function of transverse momentum and centrality. A large dependence on the pseudorapidity gap is found. Results are compared with other experiments and model calculations.en_US
dc.language.isoenen_US
dc.publisherPhysical Review C - Nuclear Physicsen_US
dc.titleThird harmonic flow of charged particles in Au + Au collisions at √sNN = 200 GeVen_US
dc.typeArticleen_US
Appears in Collections:Journal Papers

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