Radiation reaction in the classical relativistic St rmer problem

arXiv:2608.03310 · physics.plasm-ph, astro-ph.HE, gr-qc · Submitted 2026-08-04 · Read on arXiv

Francisco S. N. Lobo, Tiberiu Harko

physics.plasm-ph, astro-ph.HE, gr-qc

Submitted: 2026-08-04

Comments: 16 pages, 2 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Benchmark — 8× in this paper · explained in 2 episodes
• Initial Data — 5× in this paper · explained in 2 episodes
• Accuracy — 2× in this paper · explained in 1 episode
• Adiabatic Evolution — 2× in this paper · explained in 2 episodes

Sources

• Exact solutions, trajectories and radiation patterns in the classical relativistic St\"{o}rmer problem
• Extremely high-intensity laser interactions with fundamental quantum systems
• Relativistic van Allen belts in magnetospheres of pulsars and white dwarfs
• Particle acceleration and radiation reaction in a strongly magnetized rotating dipole
• Particle motion in neutron stars ultra-strong electromagnetic field: the influence of radiation reaction
• Radiative Back-Reaction on Charged Particle Motion in the Dipole Magnetosphere of Neutron Stars
• Modeling high-energy pulsar lightcurves from first principles
• Ab-initio pulsar magnetosphere: three-dimensional particle-in-cell simulations of axisymmetric pulsars

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