Transport and Magnetohydrodynamics Meeting

We consider the thermodynamic properties of a rotating gas of fermions. We begin by constructing the thermodynamic potential $\Phi$ and its associated current $\phi^{\mu}$ within the grand canonical ensemble of a macroscopic rigidly rotating body, where the ensemble parameters are the temperature $T_0$ and chemical potential $μ_0$ on the rotation axis, as well as the rotation angular velocity $\Omega_0$. We then consider the problem of local thermodynamics, where the thermodynamic state is defined by the local temperature $T$ and chemical potential $\mu$, as well as the local spin potential tensor, $\Omega^{\mu \nu}$. We find the thermodynamic pressure $P$, given as the sum of the usual classical (non-quantum) and other corrections due to the spin potential and the kinematic state of the fluid. We compute the associated entropy, charge and spin densities, and show that they are consistent with the Euler relation.

Based on arXiv:2509.17640v1 [hep-th]