  We discuss the effects of strong gravity on the polarization properties of a
black hole accretion disc. The intrinsic polarization is computed taking into
account light scattered on the disc surface and using different approximations.
The gravitational field of a black hole influences the Stokes parameters of
reflected radiation propagating to a distant observer. The lamp-post model is
explored as an example of a specific geometrical arrangement relevant for AGNs.
The degree and the angle of polarization are computed as functions of the
observer inclination angle, of the inner radius of the disc emitting region,
and of other parameters of the model. The expected polarization should be
detectable by new generation polarimeters. This contribution extends results
reported in our recent paper (MNRAS 355, 1005; 2004).
