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In this paper, we study tidal forces in the Schwarzschild black hole whose metric includes explicitly a generalized uncertainty principle (GUP) effect. We also investigate interesting features of the geodesic equations and tidal effects dependent on the GUP parameter related to a minimum length. Then, by solving geodesic deviation equations explicitly with appropriate boundary conditions, we show that in the effective metric affects both the radial and angular components of the geodesic equation, particularly near the singularities.
Hong et al. (Wed,) studied this question.