particles, reaching close to the zero-mass ultrarelativistic regime treated in the previous
literature. Starting from an expansion of the Maxwell-Jüttner distribution on orthogonal
polynomials, we perform a Gauss-type quadrature procedure and discretize the relativistic
Boltzmann equation on space-filling Cartesian lattices. The model is validated through
numerical comparison with standard tests and solvers in relativistic fluid dynamics such as …