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Abstract In this analysis, we examine the angular distribution of low-mass dimuon pairs produced in simulated electron–positron collisions at the proposed International Linear Collider (ILC), which operates at a center-of-mass energy of 500 GeV and has an integrated luminosity of 4 ab^-1. Our focus is on the ₂ₒ variable, which is defined in the Collins–Soper frame. In the Standard Model, the production of low-mass dimuon pairs is primarily driven by the Drell–Yan process, which exhibits a notable forward–backward asymmetry. However, many scenarios beyond the Standard Model predict different shapes for the ₂ₒ distribution. This angular distribution can be valuable for distinguishing between these models, especially in the event of observing excesses beyond the Standard Model expectations. We utilized the mono-Z^ model to interpret the simulated data. In the absence of any discoveries of new physics, we establish upper limits at the 95% confidence level on the masses of various particles in the model, which includes the spin-1 Z^ boson and fermionic dark matter.
S. Elgammal (Mon,) studied this question.