Hawking Radiation and Black Hole Evaporation: Adaptive Time-Step Numerical Modeling and Cosmic-Scale Analysis (Simulation Code and Datasets)

This repository contains the Python simulation software and datasets developed for modeling black hole thermal radiation and the evaporation process based on Quantum Field Theory (QFT) and General Relativity. Using an adaptive time-step 4th-order Runge-Kutta (RK4) algorithm, the simulation tracks mass loss and Hawking temperature across four distinct mass regimes (from micro to supermassive black holes). The physical background includes the Schwarzschild metric, Bekenstein-Hawking entropy, greybody factors, and the thermodynamic implications of the Cosmic Microwave Background (CMB) barrier.