  We investigate tidal effects produced in the spacetime of Schwarzschild black
hole in holographic massive gravity, which has two additional mass parameters
due to massive gravitons. As a result, we have obtained that massive gravitons
affect the angular component of the tidal force, while the radial component has
the same form with the one in massless gravity. On the other hand, by solving
the geodesic deviation equations, we have found that radial components of two
nearby geodesics keep tightening while falling into the black hole and after
passing the event horizons get abruptly infinitely stretched due to massive
gravitons. However, angular components of two nearby geodesics get stretched
firstly, reach a peak and then get compressed while falling into the black
hole. Moreover, we have also shown that the angular components are more easily
deformed near the departure position as the mass of a black hole is smaller for
a fixed graviton mass.

General Relativity and Quantum Cosmology