Quantization of the interior of the black hole

Abstract

In this work we study the Schwarzschild metric in the context of canonical quantum gravity inside the horizon, close of horizon and near the black hole singularity. Using this standard quantization procedure, we show that the horizon is quantized and the black hole singularity disappears. For the first case, quantization of the Schwarzschild radius was obtained in terms of the Planck length $l_{Pl}$, a positive integer $n$ and the ordering factor of the operator $p$. From the quantization of the Schwarzschild radius it was possible to determine the area of the black hole event horizon, its mass and the quantum energy of the Hawking radiation as well as its frequency. For the solution close to the interior black hole singularity, the wave function was determined and applied the DeBroglie-Bohm interpretation. The Bohm's trajectory was found near to the singularity. It which describes how the spacetime evolves over time and depends on the ordering factor of the operator $p$. Thus, for the case where $|1-p|\ne 0,3$, the Bohm's trajectory is finite and regular, that is, the singularity is removed. For the case where $|1-p|=3$, the Bohm's trajectory assumes an exponential behavior, never going to zero, avoiding the singularity.That result allows that spacetime be extended beyond the classical singularity.

References in corpus (15)

• Disappearance of Black Hole Singularity in Quantum Gravity
• The Causal Interpretation of Dust and Radiation Fluids Non-Singular Quantum Cosmologies
• Canonical Quantum Gravity
• Spontaneous creation of the universe from nothing
• Singularities and Classical Limit in Quantum Cosmology
• Spherically symmetric canonical quantum gravity
• 2+1 dimensional magnetically charged solutions in Einstein - Power - Maxwell theory
• Quantum singularity of Levi-Civita spacetimes
• Quantum Singularities Around a Global Monopole
• Quantum singularities in the BTZ spacetime
• Quantum singularities in (2+1) dimensional matter coupled black hole spacetimes
• Quantum Singularities in Spacetimes with Spherical and Cylindrical Topological Defects
• On the factor ordering problem in stochastic inflation
• Quantum singularities in static and conformally static space-times
• Quantum singularities in a model of f(R) Gravity