Statistical thermodynamics of a two dimensional relativistic gas

In this article we study a fully relativistic model of a two dimensional hard-disk gas. This model avoids the general problems associated with relativistic particle collisions and is therefore an ideal system to study relativistic effects in statistical thermodynamics. We study this model using molecular-dynamics simulation, concentrating on the velocity distribution functions. We obtain results for $x$ and $y$ components of velocity in the rest frame ($\Gamma$) as well as the moving frame ($\Gamma'$). Our results confirm that J\"{u}ttner distribution is the correct generalization of Maxwell-Boltzmann distribution. We obtain the same "temperature" parameter $\beta$ for both frames consistent with a recent study of a limited one-dimensional model. We also address the controversial topic of temperature transformation. We show that while local thermal equilibrium holds in the moving frame, relying on statistical methods such as distribution functions or equipartition theorem are ultimately inconclusive in deciding on a correct temperature transformation law (if any).