Abstract

We derive the relativistic non-resistive, viscous second-order magnetohydrodynamic equations for the dissipative quantities using the relaxation time approximation. The Boltzmann equation is solved for a system of particles and antiparticles using Chapman-Enskog like gradient expansion of the single-particle distribution function truncated at second order. In the first order, the transport coefficients are independent of the magnetic field. In the second-order, new transport coefficients that couple magnetic field and the dissipative quantities appear which are different from those obtained in the 14-moment approximation [1] in the presence of a magnetic field. However, in the limit of the weak magnetic field, the form of these equations are identical to the 14-moment approximation albeit with different values of these coefficients. We also derive the anisotropic transport coefficients in the Navier-Stokes limit.

Highlights

  • Stages of heavy-ion collisions at Relativistic Heavy Ion Collider (RHIC) near Brookhaven, New York and at Large Hadron Collider (LHC) near Geneva, Switzerland

  • We derive for the first time the relativistic non-resistive, viscous second-order magnetohydrodynamics equations for the dissipative quantities using the relaxation time approximation

  • Assuming that the single-particle distribution function is close to equilibrium, we solve the Boltzmann equation in the presence of a magnetic field using Chapman-Enskog like gradient expansion with two relevant expansion parameters: the Knudsen number and a dimensionless parameter χ = qBτc/T that depends on the strength of the magnetic field

Read more

Summary

Equations of motion of the electromagnetic field

We start by giving some text-book like introduction to the relativistically covariant formulation of electrodynamics. Where Jν is the electric charge four-current which acts as the source of electromagnetic field It can be tensor decomposed in a fluid with four velocity uμ in the following manner:. The induced charge density due to the electromagnetic field Jiμnd = σEμ (here σ is the isotropic electrical conductivity i.e., σμν = σgμν) has to be finite, so to maintain that Eμ → 0 for this case. This brings our electromagnetic tensor F μν to the following form: Fμν → Bμν = μναβ uαBβ.

Kinetic theory and hydrodynamics
Conservation of energy-momentum tensor of fluid and field
Ideal and dissipative non-resistive magnetohydrodynamics
Boltzmann equation
Expansion in gradients
First order equations
Second order equations
The ultrarelativistic and weak field limit
The Navier-Stokes limit
Conclusion
A Thermodynamic integrals
B Second order relaxation equation for dissipative stresses
Bulk stress
Diffusion current
C Projection tensors
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call