# Evolution of three-dimensional Relativistic Ion Weibel Instability: Competition with Kink Instability

## TL;DR

This paper investigates the nonlinear behavior of the relativistic Weibel instability in collisionless plasmas through simulations, revealing its stability against kink instability and its potential to generate seed magnetic fields for MHD dynamos.

## Contribution

It provides a detailed analysis of the nonlinear saturation of the relativistic Weibel instability and demonstrates its stability against kink instability in the MHD regime, supporting its role in magnetic field generation.

## Key findings

- Weibel instability's nonlinear phase characterized by filament current densities.
- Relativistic kink instability does not affect Weibel filaments up to 1000 ω_{p,i}^{-1}.
- Stable magnetic fields from Weibel instability can seed MHD dynamos.

## Abstract

In this paper, we report our recent findings on the relativistic Weibel instability and its nonlinear saturation by performing numerical simulations of collisionless plasmas. Analysis of the obtained numerical results revealed that the nonlinear phase of the Weibel instability can be described by characteristic phases based on the Weibel filaments' current density in terms of particle and Alfv\'en limit currents. We also analyzed the relativistic kink instability based on the energy principle in the magnetohydrodynamic (MHD) regime, and found that the Weibel filaments do not suffer from the kink-type instability in the MHD regime up to 1000 $\omega_{p,i}^{-1}$. This finding allowed a magnetic field to be sustained by relativistic Weibel instability that was stable enough to be a seed for MHD dynamos.