analiza aiqbench

This research redefines black hole singularities from zero-dimensional points to three-dimensional surfaces using General Relativity simulations of falling observers. By resolving a causal paradox where separated astronauts cannot meet, the study suggests that non-rotating black holes possess an expansive central structure rather than a single point of infinite density. This theoretical shift has significant implications for our understanding of spacetime geometry and event horizons in extreme gravitational environments.