Radiative polarization dynamics of relativistic electrons in an intense electromagnetic field

TL;DR

This paper introduces a comprehensive, self-consistent model for simulating the evolution of relativistic electron spin polarization in intense electromagnetic fields, improving accuracy and efficiency over previous models.

Contribution

The authors develop a novel Monte Carlo simulation method that incorporates radiative polarization dynamics and precession, extending the polarization vector model to complex laser plasma environments.

Findings

Successfully reproduces the Sokolov-Ternov effect

Demonstrates superior accuracy and efficiency

Applicable to laser plasma interaction simulations

Abstract

We propose a self-consistent model which utilizes the polarization vector to theoretically describe the evolution of spin polarization of relativistic electrons in an intense electromagnetic field. The variation of radiative polarization due to instantaneous no photon emission is introduced into our model, which extends the applicability of the polarization vector model derived from the nonlinear Compton scattering under local constant crossed-field approximation to the complex electromagnetic environment in laser plasma interaction. According to this model, we develop a Monte Carlo method to simulate the electron spin under the influence of radiation and precession simultaneously. Our model is consistent with the quantum physical picture that spin can only be described by a probability distribution before measurement, and it contains the entire information on the spin. The correctness of our model is confirmed by the successful reproduction of the Sokolov-Ternov effect and the comparison of the simulation results with other models in the literature. The results show the superiority in accuracy, applicability, and computational efficiency of our model, and we believe that our model is a better choice to deal with the electron spin in particle-in-cell simulation for laser plasma interaction.