  The nonlinear transport features of inhomogeneous chiral plasma in the
presence of electromagnetic fields, in rotating coordinates are studied within
the relaxation time approach. The chiral distribution functions up to second
order in the electric field in rotating coordinates and the derivatives of
chemical potentials are established by solving the Boltzmann transport
equation. First, the vector and axial current densities in the weakly ionized
chiral plasma for vanishing magnetic field are calculated. They involve the
rotational analogues of the Hall effect as well as several new terms arising
from the Coriolis and fictitious centrifugal forces. Then in the short
relaxation time regime the angular velocity and electromagnetic fields are
treated as perturbations. The current densities are obtained by retaining the
terms up to second order in perturbations. The time evolution equations of the
inhomogeneous chemical potentials are derived by demanding that collisions
conserve the particle number densities.
