  Schwarzschild black hole is the simplest black hole that is studied most in
detail. Its behavior is best understood by looking at the geodesics of the
particles under the influence of its gravitational field. In this paper, the
focus of attention is giving a perspicuous description of the Schwarzschild
geodesics by using analogue potential approach. Specifically we discuss
geodesics of light and of a massive particle in the case that their angular
momentum is non zero in the Schwarzschild spacetime. This discussion is done by
defining analogue potentials out of geodesic equations and defining relevant
dimensionless conserved quantities. Then, we designate how geodesics change in
response to the change of these quantities. Our results indicate the relation
between the particles' motion near black hole horizon and their angular
momentum. Furthermore, we make a comparison between Newtonian Physics (NP) and
General Relativity (GR) in the language of the analogue potential approach.
