The generation of magnetic fields by the Biermann battery and the interplay with the Weibel instability

TL;DR

This paper investigates magnetic field generation in plasma bubbles via the Biermann battery and Weibel instability, revealing their interplay, dependence on system size, and spectral characteristics of resulting magnetic and electric fields.

Contribution

It demonstrates how large-scale magnetic fields are generated by the Biermann battery and how the Weibel instability contributes at larger system sizes, with detailed spectral analysis.

Findings

Large-scale magnetic fields form with plasma beta near 1 when system size is comparable to ion inertial length.

The Weibel instability generates magnetic fields at larger sizes with specific wavenumber characteristics.

Magnetic and electric energy spectra follow power laws with indices -16/3 and -7/3 at sub-electron Larmor scales.

Abstract

An investigation of magnetic fields generated in an expanding bubble of plasma with misaligned temperature and density gradients (driving the Biermann battery mechanism) is performed. With gradient scales $L$, large-scale magnetic fields are generated by the Biermann battery mechanism with plasma $\beta \sim 1$, as long as $L$ is comparable to the ion inertial length $d_i$. For larger system sizes, $L/d_e > 100$ (where $d_e$ is the electron inertial length), the Weibel instability generates magnetic fields of similar magnitude but with wavenumber $k d_e \sim 0.2$. In both cases, the growth and saturation of these fields have a weak dependence on mass ratio $m_i/m_e$, indicating electron mediated physics. A scan in system size is performed at $m_i/m_e = 2000$, showing agreement with previous results with $m_i/m_e = 25$. In addition, the instability found at large system sizes is quantitatively demonstrated to be the Weibel instability. Furthermore, magnetic and electric energy spectra at scales below the electron Larmor radius are found to exhibit power law behavior with spectral indices $-16/3$ and $-7/3$, respectively.