Table of Contents
Fetching ...

From kinetic theory to dissipative fluid dynamics

B. Betz, D. Henkel, D. H. Rischke

TL;DR

The paper addresses how to obtain a causal, stable relativistic dissipative hydrodynamics framework from kinetic theory by deriving the Israel-Stewart equations from the Boltzmann equation using Grad's 14-moment expansion, keeping terms up to second order in the Knudsen number $K$. The authors show that, beyond the familiar NS terms, additional second-order contributions arise, with coefficients that depend on the chosen reference frame, and they demonstrate that the full IS equations apply to non-conformal systems with net charge density. These results extend previous IS and Muronga treatments by including new second-order terms and clarifying their kinetic-theory origin, laying groundwork for accurate, frame-dependent simulations of heavy-ion collision dynamics. The work enables more reliable phenomenology and motivates future multi-species generalizations and numerical implementations for realistic modeling of relativistic fluids.

Abstract

We present the results of deriving the Israel-Stewart equations of relativistic dissipative fluid dynamics from kinetic theory via Grad's 14-moment expansion. Working consistently to second order in the Knudsen number, these equations contain several new terms which are absent in previous treatments.

From kinetic theory to dissipative fluid dynamics

TL;DR

The paper addresses how to obtain a causal, stable relativistic dissipative hydrodynamics framework from kinetic theory by deriving the Israel-Stewart equations from the Boltzmann equation using Grad's 14-moment expansion, keeping terms up to second order in the Knudsen number . The authors show that, beyond the familiar NS terms, additional second-order contributions arise, with coefficients that depend on the chosen reference frame, and they demonstrate that the full IS equations apply to non-conformal systems with net charge density. These results extend previous IS and Muronga treatments by including new second-order terms and clarifying their kinetic-theory origin, laying groundwork for accurate, frame-dependent simulations of heavy-ion collision dynamics. The work enables more reliable phenomenology and motivates future multi-species generalizations and numerical implementations for realistic modeling of relativistic fluids.

Abstract

We present the results of deriving the Israel-Stewart equations of relativistic dissipative fluid dynamics from kinetic theory via Grad's 14-moment expansion. Working consistently to second order in the Knudsen number, these equations contain several new terms which are absent in previous treatments.

Paper Structure

This paper contains 10 sections, 9 equations.