Collision energy and system size dependence of longitudinal flow decorrelation in heavy-ion collisions at RHIC energies

TL;DR

This study uses a multi-phase transport model to analyze how collision energy and system size affect longitudinal flow decorrelation in heavy-ion collisions, revealing energy-dependent scaling behaviors.

Contribution

It introduces a detailed investigation of longitudinal flow decorrelation components and their dependence on collision energy and system size using the AMPT model.

Findings

Both $r_n(\eta)$ and $R_n(\eta)$ decrease linearly with pseudorapidity.

Decorrelations exhibit a power-law scaling with collision energy, $F_n \propto \log \sqrt{s_{NN}}$.

Results enhance understanding of initial geometry fluctuations in heavy-ion collisions.

Abstract

In heavy-ion collisions, the initial collision geometry and its fluctuations drive the collective expansion of final-state hadrons in the transverse plane. However, longitudinal fluctuations induce event-plane twist and flow magnitude asymmetries, collectively known as longitudinal flow decorrelation. Using a multi-phase transport (AMPT) model, we systematically investigate the dependence of collision energy and system size of this phenomenon with Au+Au collisions at $\sqrt{s_{\mathrm{NN}}}$ = 19.6, 27, 54.4, 200 GeV and isobar collisions (Zr+Zr and Ru+Ru) at $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV. The results reveal two distinct decorrelation components: $r_n(\eta)$, which includes flow magnitude asymmetry and event-plane twist, and $R_n(\eta)$ which arises purely from event-plane twist. Both $r_n(\eta)$ and $R_n(\eta)$ decrease linearly with $\eta$ and exhibit a significant dependence on collision energy and the size of the system. Through the slope parameters $F_n$ in the linear parametrization $r_n(\eta) = 1-2F_n\eta$, we can quantify the strength of decorrelation. We further observe that both $F_2$ and $F_3$ demonstrate a pronounced power-law scaling behavior with collision energy, following the relation $F_n \propto log \sqrt{s_{NN}}$. These results provide valuable insights into the three-dimensional modeling of the initial stage and the evolution of relativistic heavy-ion collisions.