EventsThe 1st International Online Conference on Symmetry
Published
This submission belongs to the session S3. Applied Physics of the event The 1st International Online Conference on Symmetry
Published date
15 Oct, 2026
Academic Editor
author-avatarJoao Pacheco B.C. de Melo
Citation
Nikolai Sergeevich Akintsov, Qinghua Qin, Artem Pavlovich Nevecheria, Stepan Nikolaevich Andreev, Symplectic Symmetry Preservation in Relativistic Particle Dynamics via Physics-Informed Neural Network Integrators, in Proceedings of The 1st International Online Conference on Symmetry, 20 October–22 October 2026, MDPI: Basel, Switzerland
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Symplectic Symmetry Preservation in Relativistic Particle Dynamics via Physics-Informed Neural Network Integrators

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1. Research Center for Intelligent Information Technology, Nantong University, Nantong, China
2. Institute of Advanced Interdisciplinary Technology (IAIT), Shenzhen MSU-BIT University, Shenzhen 518172, China
3. Department of Mathematical and Computer Methods, Kuban State University, Krasnodar 350040, Russia
4. Joint-stock company "Center for Research and Development", Milyutinsky Lane 13, Moscow 101000, Russia
Abstract

The long-term numerical integration of relativistic charged particle dynamics in intense laser-plasma fields poses a fundamental challenge: conventional explicit integrators break the symplectic symmetry of the underlying Hamiltonian structure, leading to systematic energy drift over extended simulation times. This symmetry violation reflects a failure to preserve the phase-space geometry dictated by Liouville's theorem and the canonical Poisson bracket structure of relativistic mechanics.

We present a physics-informed neural network (PINN) framework explicitly designed to enforce symplectic symmetry as a hard architectural constraint. The network is trained to approximate the flow map of the relativistic Hamiltonian system, with the symplectic condition incorporated directly into the loss functional alongside the equations of motion residuals and initial condition penalties. This approach preserves the time-reversal and area-preserving symmetries of Hamiltonian dynamics by construction, in contrast to standard PINN formulations where physical constraints are imposed only softly. The method is validated for relativistic electrons in the fields of plane monochromatic waves and ultrashort pulsed laser beams, using rapidity-spectral Lorentz coordinates as the dynamical variables. Energy conservation errors are compared across classical integrators, standard symplectic methods, and the proposed PINN-symplectic scheme over timescales spanning many oscillation periods. The PINN-symplectic integrator demonstrates bounded energy error growth consistent with near-conservation of the modified Hamiltonian, outperforming both standard PINN and explicit Runge–Kutta approaches. These results demonstrate that embedding continuous symmetry principles into neural network architectures yields physically consistent, long-time-stable simulations of relativistic systems — a finding of direct relevance to laser-driven particle acceleration, spin-polarized beam modeling, and relativistic plasma diagnostics at next-generation facilities.

Keywords
symplectic integrators
physics-informed neural networks
Hamiltonian symmetry
relativistic particle dynamics
laser-plasma interaction
energy conservation
Lorentz coordinates
rapidity parametrization
machine learning in physics
charged particle sim
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