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In this paper we study the geodesic structure of the Schwarzschild black holein rainbow gravity analyzing the behavior of null and time-like geodesic. Wefind that the structure of the geodesics essentially does not change when thesemi-classical effects are included. However, we can distinguish differentscenarios if we take into account the effects of rainbow gravity. Depending onthe type of rainbow functions under consideration, inertial and externalobservers see very different situations in radial and non radial motion of atest particles.

Geodesic Structure of the Schwarzschild Black Hole in Rainbow Gravity