  The interstellar medium of the radio galaxy IC 5063 is highly perturbed by an
AGN jet expanding in the gaseous disc of the galaxy. We model this interaction
with relativistic hydrodynamic simulations and multiphase initial conditions
for the interstellar medium and compare the results with recent observations.
As the jets flood through the inter-cloud channels of the disc, they ablate,
accelerate, and disperse clouds to velocities exceeding $400 \mbox{km s}^{-1}$.
Clouds are also destroyed or displaced in bulk from the central regions of the
galaxy. Our models with jet powers of $10^{44} \mbox{erg s}^{-1}$ and $10^{45}
\mbox{erg s}^{-1}$ are capable of reproducing many of the features seen in the
position-velocity diagram published in Morganti et al. (2015) and confirm the
notion that the jet is responsible for the strongly perturbed gas dynamics seen
in the ionized, neutral, and molecular gas phases. In our simulations, we also
see strong venting of the jet plasma perpendicular to the disc, which entrains
clumps and diffuse filaments into the halo of the galaxy. Our simulations are
the first 3D hydrodynamic simulations of the jet and ISM of IC 5063.
