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.
Highlights
In collider-based high-energy physics, parton, particle, and detector-level Monte Carlo (MC) simulation programs enable scientific inference by connecting fundamental theories to observable quantities
To illustrate the potential of DCTR, full phase-space reweighting and parameter tuning is performed on a sample of generated events from the PYTHIA 8.230 [57,58] event generator
The jets are presented to the neural network for training, with each jet constituent represented by ðpT; η; φ; particle type; θÞ, where θ is the parameter in Eq (2)
Summary
In collider-based high-energy physics, parton-, particle-, and detector-level Monte Carlo (MC) simulation programs enable scientific inference by connecting fundamental theories to observable quantities. These tools are often computationally slow and emulate probability distributions that are analytically intractable. This has resulted in three key simulation challenges for particle physics: (1) an insufficient number of simulated events, (2) unaccounted for biases from simulation parameters, and (3) the inability to utilize all kinematic and flavor information (“the full phase space”) for parameter tuning.
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