Gravitational effects of condensed dark matter on strange stars
  In the present work we study the gravitational effects of condensed dark
matter on strange stars. We consider self-interacting dark matter particles
with properties consistent with current observational constraints, and dark
matter inside the star is modelled as a Bose-Einstein condensate. We integrate
numerically the Tolman-Oppenheimer-Volkoff equations in the two-fluid formalism
assuming that strange stars are made of up to 4 per cent of dark matter. It is
shown that for a mass of the dark matter particles in the range $50 MeV-160
MeV$ strange stars are characterized by a maximum mass and radius similar to
the ones found for neutron stars.
