Geodesic motion around a supersymmetric black hole

In this article the geodesic motion of test particles in the spacetime of a supersymmetric black hole is studied. The equations of motion are derived and solved in terms of the Weierstrass , , and functions. Effective potentials and parametric diagrams are used to analyze and characterize timelike, lightlike, and spacelike particle motion and a list of possible orbit types is given. Furthermore, various plots of orbits are presented.