Year: 2008
Type: conference-paper
Abstract: We continue the study of spherically symmetric vacuum space‐times in loop quantum gravity by treating the interior of a black hole. We start from a midi‐superspace approach, but a simple gauge fixing leads to a Kantowski–Sachs form for the variables. We show that one can solve the quantum theory exactly in the (periodic) connection representation, including the inner product. The evolution can be solved exactly by de‐parameterizing the theory and can be easily interpreted as a semi‐classical evolution plus quantum corrections. A relational evolution can also be introduced in a precise manner, suggesting what may happen in situations where it is not possible to de‐parameterize. We show that the singularity is replaced by a bounce at which quantum effects are important and that the extent of the region at the bounce where one departs from classical general relativity depends on the initial data.
Source: AIP conference proceedings
DOI: 10.1063/1.2902798
Authors: Miguel Campiglia, Rodolfo Gambini, Jorge Pullin, Alfredo Macias, Claus Lämmerzahl, Abel Camacho
Language: English
Subfield: Statistical and Nonlinear Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W1563255518