Search for the Chiral Magnetic Wave with Anisotropic Flow of Identified Particles at RHIC-STAR

The chiral magnetic wave (CMW) has been theorized to propagate in the Quark-Gluon Plasma formed in high-energy heavy-ion collisions. It could cause a finite electric quadrupole moment of the collision system, and may be observed as a dependence of elliptic flow, $v_2$, on the asymmetry between positively and negatively charged hadrons, $A_{\mathrm{c}\mathrm{h}}$. However, non-CMW mechanisms, such as local charge conservation (LCC) and hydrodynamics with isospin effect, could also contribute to the experimental observations. Here we present the STAR measurements of elliptic flow $v_2$ and triangular flow $v_3$ of charged pions, along with $v_2$ of charged kaons and protons, as functions of $A_{\rm ch}$inAu+Aucollisionsat$\sqrt{s_{\rm NN}}$ = 200 GeV. The slope parameters of $\mathrm{\Delta }{v}_2$($A_{\mathrm{c}\mathrm{h}}$) and $\mathrm{\Delta }{v}_3$($A_{\mathrm{c}\mathrm{h}}$) are reported and compared to investigate the LCC background. The similarity between pion and kaon slopes suggests that the hydrodynamics is not the dominant mechanism. The difference between the normalized $\mathrm{\Delta }{v}_2$ and $\mathrm{\Delta }{v}_3$ slopes, together with the small slopes in p+Au and d+Au collisions at $\sqrt{s_{\rm NN}}$ = 200 GeV, suggest that the CMW picture remains a viable interpretation at RHIC.