Turbulent Magnetogenesis and Large-scale Magnetic Dynamo Amplification in Ion--electron Plasmas

arXiv:2607.04437 · physics.plasm-ph, astro-ph.CO, astro-ph.GA, astro-ph.SR · Submitted 2026-07-05 · Read on arXiv

Fabio Bacchini, Francesco Pucci, Sergio Servidio, Francesco Valentini, William H. Matthaeus

physics.plasm-ph, astro-ph.CO, astro-ph.GA, astro-ph.SR

Submitted: 2026-07-05

License: http://creativecommons.org/licenses/by/4.0/

The gist: Using fully kinetic simulations that capture unprecedentedly large (from electron to ion) scales, we study magnetogenesis driven by continuous large-scale forcing until nonlinear dynamo saturation.

Terminology

Abstract

Using fully kinetic simulations that capture unprecedentedly large (from electron to ion) scales, we study magnetogenesis driven by continuous large-scale forcing until nonlinear dynamo saturation. We uncover a two-stage mechanism in collisionless ion-electron plasmas whose dynamics diverge dramatically from the pair-plasma case. In the first phase, electron pressure anisotropy triggers electron-Weibel modes, seeding small-scale magnetic fields. Then, a second growth phase emerges when the more massive ions develop their own strong anisotropy and drive ion-Weibel-type modes; concurrently, a Biermann-battery mechanism contributes to amplifying the magnetic field. This combined dynamics provides a tenfold amplification of the magnetic field in comparison to the pair-plasma case. Over long times, dynamo action continues until the system reaches a statistical steady state. This self-consistent kinetic mechanism provides a plausible explanation for robust magnetogenesis wherever an external forcing continuously stirs the plasma.

Sources

Related papers