A relativistic WebGL simulation rendering a rotating black hole and spiraling orbital bodies in real time.

Built around Runge-Kutta 4 geodesic integration and a fully decoupled Store-to-EventBus pipeline that isolates the WebGL render loop from React state updates. Performance is sustained through precalculated conserved angular momentum per ray, adaptive step sizing, and continuous line-segment intersections to guarantee a fluid, high-frame-rate event horizon.