On the double-adiabatic equations in the relativistic regime

TL;DR

This paper extends the double-adiabatic equations to relativistic regimes, providing analytical and numerical solutions for plasma pressure evolution relevant to astrophysical phenomena involving high-energy particles.

Contribution

It introduces a relativistic extension of the double-adiabatic equations, deriving analytical solutions and validating them with kinetic simulations for high-energy astrophysical plasmas.

Findings

Analytical expressions for pressure evolution in ultrarelativistic plasmas.

Numerical solutions for relativistic double-adiabatic equations.

Validation with particle-in-cell simulations.

Abstract

We revisit the double adiabatic evolution equations and extend them to the relativistic and ultrarelativistic regimes. We analytically solve the relativistic, time-dependent drift kinetic equation for a homogeneous, magnetized, collisionless plasma and obtain a solution explicitly dependent on the magnetic field and density variations. In the case of an initial relativistic Maxwellian distribution, a natural extension to an anisotropic Maxwell-J\"uttner is obtained. We calculate the moments of this time-dependent solution and obtain analytical expressions for the evolution of the perpendicular and parallel pressures in the ultrarelativistic case. We numerically solve the moment equations in the relativistic case and obtain general expressions for the double-adiabatic equations in this regime. We confirm our results using fully kinetic particle-in-cell simulations of shearing and compressing boxes. Our findings can be readily applied to relativistic species including cosmic-rays and electron-positron pairs, present in astrophysical plasmas like pulsar wind nebulae, astrophysical jets, black hole accretion flows, and Van Allen radiation belts.