Simulations of the Biermann battery mechanism in two-fluid partially ionised plasmas
David Mart\'inez-G\'omez, Beatrice Popescu Braileanu, Elena Khomenko,, Peter Hunana

TL;DR
This study uses two-fluid simulations to explore how ionisation degree and collisional interactions influence magnetic field generation via the Biermann battery and dynamo mechanisms during Kelvin-Helmholtz instabilities in partially ionised plasmas.
Contribution
It provides new insights into the effects of ionisation and collisional processes on magnetic field generation in two-fluid plasma models during fluid instabilities.
Findings
Magnetic field generation increases with lower ionisation when collisional coupling is considered.
Charge-exchange processes slightly enhance magnetic field generation.
Results converge to single-fluid predictions at higher plasma densities.
Abstract
In the absence of an initial seed, the Biermann battery term of a non-ideal induction equation acts as a source that generates weak magnetic fields. These fields are then amplified via a dynamo mechanism. The Kelvin-Helmholtz instability is a fluid phenomenon that takes place in many astrophysical scenarios and can trigger the action of the Biermann battery and dynamo processes. We aim to investigate the effect that the ionisation degree of the plasma and the interaction between the charged and neutral species have on the generation and amplification of magnetic fields during the different stages of the instability. We use the two-fluid model implemented in the numerical code Mancha-2F. We perform 2D simulations starting from a configuration with no initial magnetic field and which is unstable due to a velocity shear. We vary the ionisation degree of the plasma and we analyse the role…
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