Responses of the chiral-magnetic-effect-sensitive sine observable to resonance backgrounds in heavy-ion collisions

Abstract

A new sine observable, R_2( S), has been proposed to measure the chiral magnetic effect (CME) in heavy-ion collisions; S = + - - , where are azimuthal angles of positively and negatively charged particles relative to the reaction plane and averages are event-wise, and R_2( S) is a normalized event probability distribution. Preliminary STAR data reveal concave R_2( S) distributions in 200 GeV Au+Au collisions. Studies with a multiphase transport (AMPT) and anomalous-viscous Fluid Dynamics (AVFD) models show concave R_2( S) distributions for CME signals and convex ones for typical resonance backgrounds. A recent hydrodynamic study, however, indicates concave shapes for backgrounds as well. To better understand these results, we report a systematic study of the elliptic flow (v2) and transverse momentum (pT) dependences of resonance backgrounds with toy-model simulations and central limit theorem (CLT) calculations. It is found that the concavity or convexity of R_2( S) depends sensitively on the resonance v2 (which yields different numbers of decay π+π- pairs in the in-plane and out-of-plane directions) and pT (which affects the opening angle of the decay π+π- pair). Qualitatively, low pT resonances decay into large opening-angle pairs and result in more `back-to-back' pairs out-of-plane, mimicking a CME signal, or a concave R_2( S). Supplemental studies of R_3( S) in terms of the triangular flow (v3), where only backgrounds exist but any CME would average to zero, are also presented.

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