A data-driven method was applied to Au+Au collisions at √sNN=200 GeV made with the STAR detector at RHIC to isolate pseudorapidity distance Δη-dependent and Δη-independent correlations by using two- and four-particle azimuthal cumulant measurements. We identified a Δη-independent component of the correlation, which is dominated by anisotropic flow and flow fluctuations. It was also found to be independent of η within the measured range of pseudorapidity |η|<1. In 20–30% central Au+Au collisions, the relative flow fluctuation was found to be 34%±2%(stat.)±3%(sys.) for particles with transverse momentum pT less than 2 GeV/c. The Δη -dependent part, attributed to nonflow correlations, is found to be 5%±2%(sys.) relative to the flow of the m...
12 pages, 12 figures ; see paper for full list of authorsWe report measurements of the third harmoni...
We present STAR measurements of various harmonics of three-particle correlations in √SNN = 200 GeV A...
We report measurements of the third harmonic coefficient of the azimuthal anisotropy, upsilon(3), kn...
A data-driven method was applied to Au+Au collisions at √sNN = 200 GeV made with the STAR detector a...
AbstractA data-driven method was applied to Au+Au collisions at sNN=200 GeV made with the STAR detec...
A data-driven method was applied to Au+Au collisions at sNN=200GeV made with the STAR detector at RH...
A data-driven method was applied to Au+Au collisions a t√s[subscript NN] = 200 GeV made with the STA...
A data-driven method was applied to Au+Au collisions at sNN=200GeV made with the STAR detector at RH...
Flow harmonics (vn) in the Fourier expansion of the azimuthal distribution of particles are widely u...
see paper for full list of authorsInternational audienceA data-driven method was applied to measurem...
Flow harmonics ($v_n$) in the Fourier expansion of the azimuthal distribution of particles are widel...
We apply a data-driven method to STAR Au+Au collisions at sNN = 200 GeV to iso-late ∆η-dependent and...
We present the first measurement of directed flow ($v_1$) at RHIC. $v_1$ is found to be consistent w...
We report measurements of the third harmonic coefficient of the azimuthal anisotropy, v[subscript 3]...
We report measurements of the third harmonic coefficient of the azimuthal anisotropy, v3, known as t...
12 pages, 12 figures ; see paper for full list of authorsWe report measurements of the third harmoni...
We present STAR measurements of various harmonics of three-particle correlations in √SNN = 200 GeV A...
We report measurements of the third harmonic coefficient of the azimuthal anisotropy, upsilon(3), kn...
A data-driven method was applied to Au+Au collisions at √sNN = 200 GeV made with the STAR detector a...
AbstractA data-driven method was applied to Au+Au collisions at sNN=200 GeV made with the STAR detec...
A data-driven method was applied to Au+Au collisions at sNN=200GeV made with the STAR detector at RH...
A data-driven method was applied to Au+Au collisions a t√s[subscript NN] = 200 GeV made with the STA...
A data-driven method was applied to Au+Au collisions at sNN=200GeV made with the STAR detector at RH...
Flow harmonics (vn) in the Fourier expansion of the azimuthal distribution of particles are widely u...
see paper for full list of authorsInternational audienceA data-driven method was applied to measurem...
Flow harmonics ($v_n$) in the Fourier expansion of the azimuthal distribution of particles are widel...
We apply a data-driven method to STAR Au+Au collisions at sNN = 200 GeV to iso-late ∆η-dependent and...
We present the first measurement of directed flow ($v_1$) at RHIC. $v_1$ is found to be consistent w...
We report measurements of the third harmonic coefficient of the azimuthal anisotropy, v[subscript 3]...
We report measurements of the third harmonic coefficient of the azimuthal anisotropy, v3, known as t...
12 pages, 12 figures ; see paper for full list of authorsWe report measurements of the third harmoni...
We present STAR measurements of various harmonics of three-particle correlations in √SNN = 200 GeV A...
We report measurements of the third harmonic coefficient of the azimuthal anisotropy, upsilon(3), kn...