  We investigate a relativistic adaptation of the Lattice Boltzmann Method that
reproduces the equations of motion for a turbulent, two-dimensional, massless
hydrodynamic system. The classical Lattice Boltzmann Method and its extension
to relativistic fluid dynamics is described. The numeric formulation is
evaluated using a zero-averaged stirring force introduced into the numerics to
induce turbulence, and the flow characteristics produced are compared to
properties of a classical turbulent hydrodynamic flow. The model can reasonably
be expected to offer quantitative simulations of electron fluid flows in
graphene or Kagome lattices.
