  In this work, we illustrate the geodesics of real particles obtained
numerically in a Regular Schwarzschild Anti-de Sitter (RSch-AdS) space-time.
The behavior of these geodesics are considered depending on variation of
effective parameters such as mass distribution, angular momentum and
cosmological constant. Also, using the laws of thermodynamics of black holes,
we will study and discuss some aspect of black hole (BH) described by this
spacetime such as temperature, entropy, heat capacity and Gibbs free energy.
