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Relativistic resistive magnetohydrodynamics for a two-component plasma

Khwahish Kushwah, Caio V. P. de Brito, Gabriel S Denicol

TL;DR

This work derives a covariant, kinetic-theory–based framework for relativistic resistive MHD in a two-component ultrarelativistic plasma by applying the 14-moment approximation to the Boltzmann–Vlasov equations in the Landau frame. It yields tightly coupled evolution equations for the net charge diffusion current $\mathcal{V}^\mu$, the total and relative diffusion currents, and the total and relative shear-stress tensors $\pi^{\mu\nu}$ and $\delta\pi^{\mu\nu}$, incorporating nonlinear feedback between electric/magnetic fields and dissipative quantities and inter-species collisions. The theory agrees with Israel–Stewart–type relaxation in the regime of small $\eta/s$, vanishing $B$, and moderate $E$, while revealing controlled deviations under strong electric fields due to back-reaction and a nonzero relative energy diffusion $\delta h^\mu$ that can generate anisotropy even without flow. Analyses of homogeneous and Bjorken-flow cases show that Ohmic relaxation is a good description at late times in neutral, homogeneous settings, whereas expansion and strong fields amplify nonlinear couplings, with diffusion and shear coupling persisting but damped in expanding geometries. This provides a kinetic-grounded, covariant description of two-component resistive MHD with potential applications to relativistic plasmas in heavy-ion collisions and astrophysical contexts.

Abstract

We derive relativistic resistive magnetohydrodynamics for a two-component ultrarelativistic plasma directly from kinetic theory. Starting with the Boltzmann--Vlasov equation and using the 14-moment approximation in the Landau frame, we obtain coupled evolution equations for the charge diffusion four-current and the shear-stress tensor. Benchmarking against the usual Israel-Stewart type relaxation form shows that this simplified description is accurate for small viscosity to entropy ($η/s$) ratio, vanishing magnetic field, and not so strong electric field. Outside this regime the dynamics depart in a controlled way, i.e., strong electric fields introduce nonlinear back-reaction that delays and reduces current peaks, and a sizable shear-stress is produced even without a flow profile.

Relativistic resistive magnetohydrodynamics for a two-component plasma

TL;DR

This work derives a covariant, kinetic-theory–based framework for relativistic resistive MHD in a two-component ultrarelativistic plasma by applying the 14-moment approximation to the Boltzmann–Vlasov equations in the Landau frame. It yields tightly coupled evolution equations for the net charge diffusion current , the total and relative diffusion currents, and the total and relative shear-stress tensors and , incorporating nonlinear feedback between electric/magnetic fields and dissipative quantities and inter-species collisions. The theory agrees with Israel–Stewart–type relaxation in the regime of small , vanishing , and moderate , while revealing controlled deviations under strong electric fields due to back-reaction and a nonzero relative energy diffusion that can generate anisotropy even without flow. Analyses of homogeneous and Bjorken-flow cases show that Ohmic relaxation is a good description at late times in neutral, homogeneous settings, whereas expansion and strong fields amplify nonlinear couplings, with diffusion and shear coupling persisting but damped in expanding geometries. This provides a kinetic-grounded, covariant description of two-component resistive MHD with potential applications to relativistic plasmas in heavy-ion collisions and astrophysical contexts.

Abstract

We derive relativistic resistive magnetohydrodynamics for a two-component ultrarelativistic plasma directly from kinetic theory. Starting with the Boltzmann--Vlasov equation and using the 14-moment approximation in the Landau frame, we obtain coupled evolution equations for the charge diffusion four-current and the shear-stress tensor. Benchmarking against the usual Israel-Stewart type relaxation form shows that this simplified description is accurate for small viscosity to entropy () ratio, vanishing magnetic field, and not so strong electric field. Outside this regime the dynamics depart in a controlled way, i.e., strong electric fields introduce nonlinear back-reaction that delays and reduces current peaks, and a sizable shear-stress is produced even without a flow profile.

Paper Structure

This paper contains 21 sections, 108 equations, 5 figures.

Figures (5)

  • Figure 1: Time evolution of the unnormalized diffusion current $\mathcal{V}_{q,x}(t)$ for different initial field strengths $E_0$, with $\eta/s = 1$, $|q| = 2/3$, and $\sigma_T = 0.1\,\sigma_T^{+-}$. Larger $E_0$ values lead to more pronounced transient peaks before relaxation. All trajectories converge to the same asymptotic limit, consistent with a steady Ohmic regime.
  • Figure 2: Normalized time evolution of $\mathcal{V}_{q,x}/E_x$ for several initial electric field strengths $E_0$, with $\eta/s = 1$, $|q| = 2/3$, and $\sigma_T = 0.1\,\sigma_T^{+-}$. At late times, all curves converge to the same asymptotic value, consistent with the Ohmic limit $\mathcal{V}_{q,x} \simeq \sigma_{\rm E}\, E_x$. The early-time deviation reflects nonlinear relaxation effects under stronger applied fields.
  • Figure 3: Time evolution of the diffusion current $\mathcal{V}_{q,x}(t)$ for different values of $\eta/s$, with fixed $|q|=1$, $\sigma_T = 0.1\,\sigma_T^{+-}$ and $E_0$ = $30\, fm^{-2}$. Increasing $\eta/s$ reduces collisional damping and gives rise to oscillatory relaxation, while smaller $\eta/s$ leads to a smooth exponential decay.
  • Figure 4: Time evolution of the normalized shear-stress component $\pi_{xx}/\epsilon$ for various $E_0$ values, with $\eta/s = 1$, $\sigma_T/\sigma_T^{+-} = 0.1$. Larger $E_0$ enhances the transient peak due to stronger field-induced anisotropy, while all curves relax to zero at late times, restoring isotropy.
  • Figure 5: Time evolution of the charge diffusion current $\mathcal{V}_{q,x}$ and normalized shear-stress $\pi_{xx}/\epsilon$ in Bjorken flow for different initial electric field strengths $E_0$. The left panel shows $\mathcal{V}_{q,x}$, exhibiting an early-time peak that increases with $E_0$ and decays slowly due to viscous and expansion damping. The right panel shows $\pi_{xx}/\epsilon$, which exhibits similar early peak trend but does not depend on $E_0$ values and thus is hugely governed by the hydrodynamical process.