Interactive simulations for Black Hole and Quantum Chaos phenomena.
Visualization of Out-of-Time-Order Correlator F(t) showing exponential chaos growth before scrambling time, then saturation.
Calculate black hole properties from its mass: Schwarzschild radius, Hawking temperature, Bekenstein-Hawking entropy, and evaporation time.
Evolution of Hawking radiation entropy. Initially rises (thermal), then falls after Page time (information exits) - demonstrating unitarity.
Visualization of horizons and ergosphere for a rotating black hole (Kerr). Spin parameter a determines the ergosphere shape.
Comparison of Lyapunov exponents across various systems with the Maldacena-Shenker-Stanford bound. Black holes (and SYK model) saturate the bound.
Quasinormal mode frequencies for Schwarzschild black hole. Real part (oscillation) and imaginary part (decay rate).
Conformal diagram for Schwarzschild black hole. Each point represents a 2-sphere. 45° lines = null geodesics (light).
Computational complexity growth for black holes. Linear growth until exponential time, then saturation (Poincaré recurrence).