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Third Harmonic Flow of Charged Particles in Au+Au Collisions at $\sqrt{; ; ; ; s_{; ; ; ; NN}; ; ; ; }; ; ; ; $ = 200 GeV (CROSBI ID 200529)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Adamczyk, L. ; ... ; Planinić, Mirko ; ... ; Poljak, Nikola ; ... ; Zyzak, M. Third Harmonic Flow of Charged Particles in Au+Au Collisions at $\sqrt{; ; ; ; s_{; ; ; ; NN}; ; ; ; }; ; ; ; $ = 200 GeV // Physical review. C, Nuclear physics, 88 (2013), 14904-1-14904-11. doi: 10.1103/PhysRevC.88.014904

Podaci o odgovornosti

Adamczyk, L. ; ... ; Planinić, Mirko ; ... ; Poljak, Nikola ; ... ; Zyzak, M.

engleski

Third Harmonic Flow of Charged Particles in Au+Au Collisions at $\sqrt{; ; ; ; s_{; ; ; ; NN}; ; ; ; }; ; ; ; $ = 200 GeV

We report measurements of the third harmonic coefficient of the azimuthal anisotropy, v_3, known as triangular flow. The analysis is for charged particles in Au+Au collisions at sqrtsNN = 200 GeV, based on data from the STAR experiment at the 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.

flow; charged; AuAu; STAR

STAR Collaboration.

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Podaci o izdanju

88

2013.

14904-1-14904-11

objavljeno

0556-2813

10.1103/PhysRevC.88.014904

Povezanost rada

Fizika

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