Abstract

Starting from the Boltzmann equation in the relaxation time approximation and employing a Chapman–Enskog like expansion for the distribution function close to equilibrium, we derive second-order evolution equations for the shear stress tensor and the dissipative charge current for a system of massless quarks and gluons. The transport coefficients are obtained exactly using quantum statistics for the phase space distribution functions at non-zero chemical potential. We show that, within the relaxation time approximation, the second-order evolution equations for the shear stress tensor and the dissipative charge current can be decoupled. We find that, for large values of the ratio of chemical potential to temperature, the charge conductivity is small compared to the coefficient of shear viscosity. Moreover, we show that in the relaxation-time approximation, the limiting behaviour of the ratio of heat conductivity to shear viscosity is qualitatively similar to that obtained for a strongly coupled conformal plasma.

Highlights

  • High-energy heavy ion collisions at the BNL Relativistic Heavy Ion Collider (RHIC) [1,2] and the CERN Large Hadron Collider (LHC) [3,4,5] create strongly interacting matter under extreme conditions of high temperature and density as it is believed to have existed in the very early universe [6,7]

  • In this Letter, we present the derivation of second-order evolution equations for shear stress tensor and dissipative charge current for a system consisting of massless quarks and gluons

  • The bulk viscous pressure vanishes for such a system and the dissipation is solely due to the shear stress tensor and the dissipative charge current

Read more

Summary

Introduction

High-energy heavy ion collisions at the BNL Relativistic Heavy Ion Collider (RHIC) [1,2] and the CERN Large Hadron Collider (LHC) [3,4,5] create strongly interacting matter under extreme conditions of high temperature and density as it is believed to have existed in the very early universe [6,7]. In the presence of conserved charges but for classical particles with vanishing masses, the second-order transport coefficients corresponding to charge diffusion (or alternatively heat conduction) have been obtained by employing the moment method [40,41]. They still remain to be determined for quantum statistics. In order to obtain the form of the non-equilibrium distribution function, we employ a Chapman–Enskog like expansion to iteratively solve the Boltzmann equation in the relaxation time approximation [32] Using this expansion, we derive the first-order constitutive relations and subsequently the second-order evolution equations for the dissipative quantities. We demonstrate that the limiting behaviour of the heat conductivity to shear viscosity ratio, obtained here in the relaxation-time approximation, is qualitatively identical to that of a conformal fluid in the strong coupling limit

Relativistic hydrodynamics
Dissipative evolution equations
Transport coefficients
Conclusions and outlook

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

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.