Prediction and Anomaly Detection of accelerated particles in PIC simulations using neural networks
Gabriel Torralba Paz, Artem Bohdan, Jacek Niemiec

TL;DR
This paper introduces neural network techniques to analyze particle trajectories in PIC simulations, enabling accurate energy prediction, classification, and anomaly detection, thereby improving understanding of particle acceleration in astrophysical plasmas.
Contribution
The paper presents a novel neural network-based approach for analyzing particle data in PIC simulations, enhancing classification, regression, and anomaly detection capabilities.
Findings
Neural networks accurately predict particle energies despite noisy data.
Classification and anomaly detection effectively distinguish energetic particles.
Method simplifies analysis of large-scale PIC simulation data.
Abstract
Acceleration processes that occur in astrophysical plasmas produce cosmic rays that are observed on Earth. To study particle acceleration, fully-kinetic particle-in-cell (PIC) simulations are often used as they can unveil the microphysics of energization processes. Tracing of individual particles in PIC simulations is particularly useful in this regard. However, by-eye inspection of particle trajectories includes a high level of bias and uncertainty in pinpointing specific acceleration mechanisms that affect particles. Here we present a new approach that uses neural networks to aid individual particle data analysis. We demonstrate this approach on the test data that consists of 252,000 electrons which have been traced in a PIC simulation of a non-relativistic high Mach number perpendicular shock, in which we observe the two-stream electrostatic Buneman instability to pre-accelerate a…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae
