  We study the effects of dark matter on the properties of neutron stars by
employing a DM-admixed model. The Brueckner-Hartree-Fock theory with realistic
three-body forces and a generic bosonic self-interacting dark matter model
describe the equations of state for nuclear matter and DM, respectively. We
study the complete set of stable dark neutron stars and in particular the
observable radii of these objects. A rich variety of stellar configurations is
found and discussed in detail.
