Strings and Things

                                                                              Black Hole Simulation                                                                                                                  This simulation demonstrates quantum spacetime fluctuations under extreme conditions , simulating a  black hole-like scenario with the following dynamics: Localized High Energy Density : The central regio...

  🚀 Developing a Quantum Tensor Model for Hawking Radiation Modification We now construct a Quantum Tensor Gravity (QTG) model to modify Hawking radiation , integrating: Quantum Tensor Oscillations into Black Hole Radiation Theory. Derivation of a Modified Hawking Temperature from Tensor Fields. Quantum Corrections to Black Hole Evaporation. Implications for the Black Hole Information Paradox. Numerical Simulation of Modified Hawking Radiation Over Time. 📖 Step 1: Standard Hawking Radiation & the Information Paradox 1.1 Classical Hawking Radiation Formula In standard General Relativity, black holes radiate energy via Hawking radiation , given by: T H = ℏ c 3 8 π G M T_H = \frac{\hbar c^3}{8\pi G M} where: T H T_H is the Hawking temperature. M M is the mass of the black hole. G G is Newton’s gravitational constant. ℏ \hbar is the reduced Planck constant. ➡ Problem: This process suggests complete evaporation , leading to information loss , which contr...