cs.LGJul 15, 2026

Mono-Z Dark Matter Search with Neural Spline Flows Using CMS Run 2015D Open Data

Authors: Hitesh RasineniBhavishya Chebrolu

Organizations: VIT-AP University, Amaravati, India · 1VIT-AP University, Amaravati, 522241, India · Mohan Babu University, Tirupati, India · 2Mohan Babu University, Tirupati, 517102, India

Abstract

We report a search for dark matter (DM) produced in association with a leptonically decaying ZZ boson at s=13\sqrt{s}=13 TeV using CMS Run 2015D open data corresponding to an integrated luminosity of 2.32fb12.32\,\mathrm{fb}^{-1} together with simplified-model Monte Carlo simulation. Events are selected in the mono-Z+Z\rightarrow\ell^+\ell^- final state in both the μμμμ and eeee channels. Forty kinematic observables are extracted from MINIAOD and MINIAODSIM, cleaned with physics-motivated selections, and reduced to a 37-dimensional feature vector. Five Neural Spline Flows are trained independently to model Standard Model background and mediator-specific DM signal densities. The per-event test statistic is constructed from the log-likelihood ratio between the signal and background density estimates, providing sensitivity across the full kinematic phase space without requiring a hard upper MET\mathrm{MET} threshold. A simultaneous profile-likelihood fit combining the two channels yields observed (expected) 95% confidence level upper limits on the signal-strength parameter of μ<0.0177μ<0.0177 (0.00180.0018) for the scalar mediator, μ<0.0362μ<0.0362 (0.00390.0039) for the vector mediator, and μ<0.0498μ<0.0498 (0.00690.0069) for the axial-vector mediator. The observed limits are weaker than expected because of a residual high-MET\mathrm{MET} background-modeling discrepancy rather than evidence for a DM signal. To our knowledge, this is the first application of Neural Spline Flow likelihood-ratio scoring to a mono-ZZ dark matter search using CMS Run 2015D open data simultaneously in the μμμμ and eeee channels.

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