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Neural Networks for Full Phase-space Reweighting and Parameter Tuning

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arxiv 1907.08209 v3 pith:HOWH6D5I submitted 2019-07-18 hep-ph hep-exstat.ML

classification hep-phhep-exstat.ML
keywords fullneuralphasereweightingsimulationsspacetuningapproach
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abstract

Precise scientific analysis in collider-based particle physics is possible because of complex simulations that connect fundamental theories to observable quantities. The significant computational cost of these programs limits the scope, precision, and accuracy of Standard Model measurements and searches for new phenomena. We therefore introduce Deep neural networks using Classification for Tuning and Reweighting (DCTR), a neural network-based approach to reweight and fit simulations using all kinematic and flavor information -- the full phase space. DCTR can perform tasks that are currently not possible with existing methods, such as estimating non-perturbative fragmentation uncertainties. The core idea behind the new approach is to exploit powerful high-dimensional classifiers to reweight phase space as well as to identify the best parameters for describing data. Numerical examples from $e^+e^-\rightarrow\text{jets}$ demonstrate the fidelity of these methods for simulation parameters that have a big and broad impact on phase space as well as those that have a minimal and/or localized impact. The high fidelity of the full phase-space reweighting enables a new paradigm for simulations, parameter tuning, and model systematic uncertainties across particle physics and possibly beyond.

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Cited by 2 Pith papers

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  1. The Well-Tempered Likelihood: Honest Confidence Intervals for Misspecified Models

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    Dividing the likelihood-ratio statistic by a goodness-of-fit statistic stops confidence intervals from collapsing under model misspecification, making them self-limit at a floor set by the model's inadequacy.

  2. Higgs Signal Strength Estimation with Machine Learning under Systematic Uncertainties

    hep-ph 2025-08 conditional novelty 6.0 of 10

    SAGE, a dual-branch GNN trained under nuisance fluctuations, estimates the Higgs signal strength with near-nominal coverage (0.662-0.683) but wider intervals than the top FAIR-HUC leaderboard methods.

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