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In this paper, we apply the classical test of general relativity on a chargedWeyl black hole, whose exterior geometry is defined by altering the sphericallysymmetric solutions of Weyl conformal theory of gravity. The tests arebasically founded on scrutinizing the angular geodesics of light rayspropagating in the gravitating system caused by the black hole. In thisinvestigation, we bring detailed discussions about the bending of light,together with two other relativistic effects, known as the Shapiro and theSagnac effects. We show that the results are in good conformity with thegeneral relativistic effects, besides giving long-distance corrections causedby the cosmological nature of the background geometry under study.

Classical tests on a charged Weyl black hole: bending of light, Shapiro delay and Sagnac effect