Medium effects on the thermal conductivity of a hot pion gas
arXiv:1403.3554 · doi:10.1103/PhysRevD.89.054013
Abstract
We investigate the effect of the medium on the thermal conductivity of a pion gas out of chemical equilibrium by solving the relativistic transport equation in the Chapman-Enskog and relaxation time approximations. Using an effective model for the pi-pi cross-section involving rho and sigma meson exchange, medium effects are incorporated through thermal one-loop self-energies. The temperature dependence of the thermal conductivity is observed to be significantly affected.
References in corpus (9)
- On the Strongly-Interacting Low-Viscosity Matter Created in Relativistic Nuclear Collisions
- Bulk viscosity of QCD matter near the critical temperature
- Bulk viscosity in quasi particle models
- Shear viscosity of a hadronic gas mixture
- QCD Viscosity to Entropy Density Ratio in the Hadronic Phase
- Investigation of Heat Conductivity in Relativistic Systems using a Partonic Cascade
- Effect of spectral modification of on shear viscosity of a pion gas
- Real-time propagators at finite temperature and chemical potential
- Transport properties of a meson gas
Cited by in corpus (8)
- Conductivity, diffusivity, and violation of Wiedemann-Franz Law in a hadron resonance gas with van der Waals interactions
- Medium effects on the relaxation of dissipative flows in a hot pion gas
- In-medium viscous coefficients of a hot hadronic gas mixture
- Medium effects on the electrical conductivity of a hot pion gas
- Thermal conductivity of hot pionic medium due to pion self-energy for and loops
- Transport Coefficients of relativistic matter: A detailed formalism with a gross knowledge of their magnitude
- Relativistic second order dissipative hydrodynamics from effective fugacity quasi particle model
- Order-by-order Anisotropic Transport Coefficients of a Magnetised Fluid: a Chapman-Enskog Approach