principle from the comparison of the acceleration of test-bodies of different composition in
Earth's gravitational field. In the present paper, we propose a test of the weak-equivalence
principle in the strong gravitational field of black holes. We construct a relativistic reflection
model in which either the massive particles of the gas of the accretion disk or the photons
emitted by the disk may not follow the geodesics of the spacetime. We employ our model to …