Flow harmonics ($\textit{v}_{n}$) of the Fourier expansion for the azimuthal distributions of hadrons are commonly employed to quantify the azimuthal anisotropy of particle production relative to the collision symmetry planes. While lower order Fourier coefficients ($\textit{v}_{2}$ and $\textit{v}_{3}$) are more directly related to the corresponding eccentricities of the initial state, the higher-order flow harmonics ($\textit{v}_{n>3}$) can be induced by a mode-coupled response to the lower-order anisotropies, in addition to a linear response to the same-order anisotropies. These higher-order flow harmonics and their linear and mode-coupled contributions can be used to more precisely constrain the initial conditions and the transport properties of the medium in theoretical models. The multiparticle azimuthal cumulant method is used to measure the linear and mode-coupled contributions in the higher-order anisotropic flow, the mode-coupled response coefficients, and the correlations of the event plane angles for charged particles as functions of centrality and transverse momentum in Au+Au collisions at nucleon-nucleon center-of-mass energy \roots = 200 GeV. The results are compared to similar LHC measurements as well as to several viscous hydrodynamic calculations with varying initial conditions.
3-particle integrated correlators
The integrated $v_{4}$ and $v_{5}$
The integrated $\chi_{4,22}$, $\rho_{4,22}$, $\chi_{5,23}$ and $\rho_{5,23}$
Recently, multiparticle-correlation measurements of relativistic $p/d/^3$He$+$Au, $p$$+$Pb, and even $p$$+$$p$ collisions have shown surprising collective signatures. Here we present beam-energy-scan measurements of 2-, 4-, and 6-particle angular correlations in $d$$+$Au collisions at $\sqrt{s_{_{NN}}}$=200, 62.4, 39, and 19.6 GeV. We also present measurements of 2- and 4-particle angular correlations in $p$$+$Au collisions at $\sqrt{s_{_{NN}}}$=200 GeV. We find the 4-particle cumulant to be real-valued for $d$$+$Au collisions at all four energies. We also find that the 4-particle cumulant in $p$$+$Au has the opposite sign as that in $d$$+$Au, indicating that the correlations are geometrical and therefore collective in origin. Further we find that the 6-particle cumulant agrees with the 4-particle cumulant in $d$$+$Au collisions at 200 GeV, which indicates that nonflow effects are subdominant and provides strong evidence of collectivity.
Components $\langle\langle$4$\rangle\rangle$ and 2$\langle\langle$2$\rangle\rangle^{2}$ and cumulant $c_2${4} = $\langle\langle$4$\rangle\rangle$ - 2$\langle\langle$2$\rangle\rangle^{2}$ as a function of $N^{FVTX}_{tracks}$. (a) and (b) show the components and cumulant, respectively, in $p$+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. (c) and (d) show the components and cumulant, respectively, in $d$+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. (b) and (d) also show the cumulant as measured in AMPT for $p$+Au and $d$+Au, respectively, indicated by the green line. The shaded green band indicates the statistical uncertainty on the AMPT values.
Components $\langle\langle$4$\rangle\rangle$ and 2$\langle\langle$2$\rangle\rangle^{2}$ and cumulant $c_2${4} = $\langle\langle$4$\rangle\rangle$ - 2$\langle\langle$2$\rangle\rangle^{2}$ as a function of $N^{FVTX}_{tracks}$. (a) and (b) show the components and cumulant, respectively, in $p$+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. (c) and (d) show the components and cumulant, respectively, in $d$+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. (b) and (d) also show the cumulant as measured in AMPT for $p$+Au and $d$+Au, respectively, indicated by the green line. The shaded green band indicates the statistical uncertainty on the AMPT values.
$v_2${2}, $v_2${2, |$\Delta\eta$| > 2}, and $v_2${4} as a function of $N^{FVTX}_{tracks}$ in $d$+Au collisions with $\sqrt{s_{NN}}$= (a) 200 GeV, (b) 62.4 GeV, (c) 39 GeV, and (d) 19.6 GeV; also shown in (a) is $v_2${6} for $\sqrt{s_{NN}}$= 200 GeV. The arrowheads on the statistical uncertainties indicate cases where the standard 1$\sigma$ uncertainty on the $c_2${4} crosses zero. For 19.6 GeV, the combined confidence interval for $v_2${4} to be real is 79%.
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