Calculation of the trajectory of a spinning particle around a black hole with an arbitrary metric tensor.

Equations of Motion from a Lagrangian of a cosmological model with fading dark matter and interacting quintessence, implemented into CLASS

A system of N interacting bodies moving in 3 dimensions over time will be simulated. The trajectories of the bodies are approximated by numerically integrating the equations of motion with the Runge-Kutta Method.

Simulation of non-uniform motion on surface