Singularities and Breaking Space-time Around Black Holes: Consequences for General Relativity and Quantum Mechanics and Elements of Black Hole Physics

Abstract

Our knowledge about space-time around black holes is based on general relativity and it is based on the 4D Minkowski-spacetime. All approaches to describe spacetime around black holes were based on the wrong assumption, that 4D space-time exists everywhere in the Universe and this leads to singularities around black holes. By solving the black hole information paradox with three corresponding theories, we arrive to the conclusion that the time dimension of the Minkowski-spacetime must end at the event horizon. This means that Minkowski-spacetime separates into spatial and time dimensions: spatial dimensions enter the black holes, while the time dimension ends (curved up) at the event horizon. The theory presented in this article explains the singularities and anomalies around black holes and is in line with the major laws of thermodynamics and gravity. The theory explains the limits of general relativity and quantum mechanics around black holes – and it also provides an explanation how we can describe black hole interiors with gravity, strong force and electric charge.