Particle dynamics in nonlinear electromagnetic waves: chaos onset, diffusive heating, and wave surfing
Maxim Lyutikov
Purdue University
physics.plasm-ph, astro-ph.HE
Submitted: 2026-07-05
License: http://creativecommons.org/licenses/by/4.0/
The gist: We investigate the dynamics of charged particles interacting with ultra-intense electromagnetic X-modes in strongly magnetized plasmas.
Terminology
Abstract
We investigate the dynamics of charged particles interacting with ultra-intense electromagnetic X-modes in strongly magnetized plasmas. We demonstrate that particle motion becomes chaotic for relative wave intensities delta = B w/B 0 0.25 (not above the field reversal threshold delta at least 1). The transition to chaos occurs via the Chirikov resonance overlap mechanism and the related destruction of Kolmogorov-Arnold-Moser (KAM) tori. The maximum Lyapunov exponent increases logarithmically with delta, even though the unmagnetized delta to infinity limit is strictly integrable. In the delta 1 regime, incomplete re-laminarization of the phase space flow leads to two distinct populations: (i) the majority of particles undergoing stochastic diffusion, and (ii) a fraction of particles that become phase-locked with the wave, experiencing macroscopic intermittent surfing (L'evy flights). The 1D Particle-In-Cell simulations using the EPOCH code in the highly magnetized (sigma 1) and under-dense regime are generally consistent with the Hamiltonian single-particle theory. The dissipation fraction of the initial EM energy remains mild.
Sources
- Explosive reconnection in magnetars
- Fast Radio Bursts from reconnection events in magnetar magnetospheres
- Radio precursors of monster shocks: a mechanism for fast radio bursts from SGR 1935+2154
- PCNN: Probable-Class Nearest-Neighbor Explanations Improve Fine-Grained Image Classification Accuracy for AIs and Humans
- Fast Radio Bursts produced during collapse of macroscopic X-mode in magnetized pair plasma
- Powerful parametric instability of Alfven waves in astrophysical pair plasma
- Relativistically Magnetized Collisionless Shocks in Pair Plasma: I. Solitons, Chaos, and Thermalization
Related papers
- Is Your AI Fast Enough to Run a Fusion Reactor?
- GyroSwin: 5D Surrogates for Gyrokinetic Plasma Turbulence Simulations
- Electromagnetic ghosts in pair plasmas
- Collisionless whistler heat-flux instability in ultra-high- beta plasmas
- Rugged magneto-hydrodynamic invariants in weakly collisional plasma turbulence: Two-dimensional hybrid simulation results
- Hybrid Fourier Neural Operator-Plasma Fluid Model for Fast and Accurate Multiscale Simulations of High Power Microwave Breakdown