Responses of the chiral-magnetic-effect-sensitive sine observable to resonance backgrounds in heavy-ion collisions
Yicheng Feng, Jie Zhao, Fuqiang Wang

TL;DR
This paper introduces a new sine observable to detect the chiral magnetic effect in heavy-ion collisions and investigates how resonance backgrounds influence its shape, revealing that flow parameters and resonance properties critically affect the observable's concavity or convexity.
Contribution
The study systematically analyzes how resonance backgrounds and flow parameters impact the new sine observable used to measure the CME, clarifying background effects.
Findings
Concavity or convexity of the observable depends on resonance $v_2$ and $p_T$.
Low $p_T$ resonances produce large opening-angle pairs mimicking CME signals.
Resonance backgrounds can produce concave shapes similar to CME signals.
Abstract
A new sine observable, , has been proposed to measure the chiral magnetic effect (CME) in heavy-ion collisions; , where are azimuthal angles of positively and negatively charged particles relative to the reaction plane and averages are event-wise, and is a normalized event probability distribution. Preliminary STAR data reveal concave distributions in 200 GeV Au+Au collisions. Studies with a multiphase transport (AMPT) and anomalous-viscous Fluid Dynamics (AVFD) models show concave 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,…
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