Code to solve Kerr and Schwarzschild Black Hole geodesics in the equator of the metrics. This code can be used to find the orbits of a time-like particle near the black holes.
For 'round' solutions in the Kerr Black Hole, use the Python script main.py to optimize for the smallest variance in radius.
The metrics are solved using standard ODE numerical methods. For the case of the Schwarzschild Black Hole, the method used is Runge-Kutta and for the Kerr Black Hole it is employed the Dormand Prince Integrator 853.