  The effects of magnetic fields on accretion disks around compact objects are
of high importance in the study of their general properties and dynamics. Here
we analyze the influence of magnetic fields on thick accretion disks around
rotating boson stars. We assume a uniform constant specific angular momentum
distribution and a polytropic equation of state. The purely hydrodynamical
thick disk solutions are extended to magnetized solutions by adding a toroidal
magnetic field and then analyzed in terms of a magnetization parameter. We
consider one-centered solutions as well as two-centered solutions and focus on
retrograde tori, since they are more distinctive due to their unique
properties. Our computed solutions indicate that strong magnetic fields
influence the characteristics of thick disks around rotating boson stars and
possibly affect their unique features.
