Optimal observables for the chiral magnetic effect from machine learning

Not scheduled
20m
Dehan Hotel(德翰大酒店)

Dehan Hotel(德翰大酒店)

No 2 Jida Road, Xiangzhou district, Zhuhai
oral

Speaker

梓谊 刘 (清华大学物理系)

Description

The chiral magnetic effect (CME) in relativistic heavy-ion collisions induces a charge separation along the magnetic field, yet its detection is obscured by large backgrounds, especially from local charge conservation (LCC). Using event-by-event AVFD simulations of Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV, we studied machine-learning strategies to enhance CME discrimination.
First, we construct observables as linear and bilinear combinations of harmonic coefficients and optimize their coefficients via gradient descent. The resulting observables suppress backgrounds to near-zero levels and improve CME sensitivity by up to 110% relative to conventional $\gamma$ correlators.
Second, by exploiting a multilayer perceptron neural network, we construct “optimal CME observables” as non-linear functions of C-even, P-even harmonic coefficients. We observe that linear combinations of P?even observables dominate the discrimination, as the network's performance (achieving ~74% classification accuracy) closely matches the theoretical sensitivity derived from linear and bilinear combinations of such observables, indicating that linear contributions are the main source of separability while nonlinear gains are marginal.
Our framework offers a systematic, interpretable route to CME detection, and the optimized observables are directly applicable to experimental data at RHIC and LHC, paving the way toward finding CME .

Primary authors

Yuji Hirono (Institute of Systems and Information Engineering, University of Tsukuba) Kazuki Ikeda (Department of Physics, University of Massachusetts Boston) Dmitri Kharzeev (Center for Nuclear Theory, Department of Physics and Astronomy, Stony Brook University) 梓谊 刘 (清华大学物理系) Shuzhe Shi (Department of Physics, Tsinghua University)

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