Relativistic Lattice Boltzmann Model with Improved Dissipation
M. Mendoza, I. Karlin, S. Succi, and H. J. Herrmann

TL;DR
This paper introduces an improved relativistic lattice Boltzmann model that accurately captures dissipative effects in ultra-relativistic hydrodynamics, validated against full Boltzmann solutions and outperforming previous models.
Contribution
The authors develop a third order moment expansion of the Maxwell-Juettner distribution and incorporate a time dilatation to enhance dissipation modeling in relativistic LB schemes.
Findings
Excellent agreement with BAMPS simulations.
More accurate than previous relativistic LB models.
Validated for high viscosity and velocities.
Abstract
We develop a relativistic lattice Boltzmann (LB) model, providing a more accurate description of dissipative phenomena in relativistic hydrodynamics than previously available with existing LB schemes. The procedure applies to the ultra-relativistic regime, in which the kinetic energy (temperature) far exceeds the rest mass energy, although the extension to massive particles and/or low temperatures is conceptually straightforward. In order to improve the description of dissipative effects, the Maxwell-Juettner distribution is expanded in a basis of orthonormal polynomials, so as to correctly recover the third order moment of the distribution function. In addition, a time dilatation is also applied, in order to preserve the compatibility of the scheme with a cartesian cubic lattice. To the purpose of comparing the present LB model with previous ones, the time transformation is also…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
