A Computational Study of the Energy Levels of Black Holes

In Cosmology, both de Sitter space and Anti-de Stter ( AdS_n) space are both named after the astrophysicist de Sitter. In Einstein's General Theory of Relativity (GR), space and time are on an equal footing, and we have a unified geometry of space-time, instead of a separate space and a separate time. This yields three cases of constantly curved space-time: de Sitter space with positive curvature; Minkowski space with zero curvature; and anti-de Sitter space with negative curvature. Very conveniently, the Anti-de Sitter space can be extended to any number of dimensions, with n representing the number of dimensions. A combination of classical General Relativity (GR) and Quantum Field Theory (QFT) provides an interesting thermodynamic description of black holes. We us an algorithm proposed by Nemati et al. (2013). In this formalism, we start with a hypercube with each of its vertices labeled with black hole binaries. The back holes are associated with probability functions, and the black holes move based on the probabilities. Our research has applications both Quantum Gravity (QG) and in Black Hole Physics (BHP).