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    Method to constrain preferential emission and spectator dynamics in heavy-ion collisions

    Vipul Bairathi1 and Somadutta Bhatta2,3,*

    • 1Instituto de Alta Investigación, Universidad de Tarapacá, Casilla 7D, Arica 1000000, Chile
    • 2Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, The Netherlands
    • 3Nikhef, Science Park 105, 1098 XG Amsterdam, The Netherlands

    • *Contact author: s.bhatta@uu.nl

    Phys. Rev. C 113, 024917 – Published 24 February, 2026

    DOI: https://doi.org/10.1103/kzyy-2wtv

    Abstract

    Longitudinal particle production in heavy-ion collisions is influenced both by preferential emission from participating nucleons and by the breakup of spectator matter, yet quantifying these effects experimentally remains challenging. We introduce a Pearson correlation between spectator and charged-particle forward-backward asymmetries as an experimental probe of these phenomena. Using Au+Au collisions at sNN=200 GeV simulated with A Multi-Phase Transport model, we validate that this correlator provides a robust, pseudorapidity-differential measure of the influence of preferential emission on the longitudinal structure of particle production. We further demonstrate that the correlation strength is sensitive to fluctuations in spectator number, which in experiments arise from evaporation and fragmentation of the spectator remnants. The proposed observable therefore offers a data-driven handle for constraining models of preferential emission and spectator breakup, thereby improving our understanding of the mechanisms that shape the final-state longitudinal distributions in heavy-ion collisions.

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