Dark Matter From f(R,T) Gravity
  We consider f(R,T) modified theory of gravity, in which the gravitational
Lagrangian is given by an arbitrary function of the Ricci scalar and the trace
of the energy-momentum tensor of the matter, in order to investigate the
dark-matter effects on the galaxy scale. We obtain the metric components for a
spherically symmetric and static spacetime in the vicinity of general
relativity solutions. However, we concentrate on a specific model of the theory
where the matter is minimally coupled to the geometry, and derive the metric
components in the galactic halo. Then, we fix the components by the rotational
velocities of the galaxies for the model, and show that the mass corresponding
to the interaction term (which appears in the Einstein modified field equation)
leads to a flat rotation curve in the halo of galaxies. In addition, for the
proposed model, the light-deflection angle has been derived and drawn using
some observed data.
