The Evolution of $Λ$ Black Holes in the Mini-Superspace Approximation of Loop Quantum Gravity

Details The Evolution of $Λ$ Black Holes in the Mini-Superspace Approximation of Loop Quantum Gravity The Evolution of $Λ$ Black Holes in the Mini-Superspace Approximation of Loop Quantum Gravity

2008-12-30

arxiv.org/abs/0901.0010v2

Phys.Rev.D79:084023,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

26 pages, 7 figures.V2 has typos corrected, references added, and a more careful analysis of the planar case. Accepted for pub

Scientific paper

10.1103/PhysRevD.79.084023

Using the improved quantization technique to the mini-superspace approximation of loop quantum gravity, we study the evolution of black holes supported by a cosmological constant. The addition of a cosmological constant allows for classical solutions with planar, cylindrical, toroidal and higher genus black holes. Here we study the quantum analog of these space-times. In all scenarios studied, the singularity present in the classical counter-part is avoided in the quantized version and is replaced by a bounce, and in the late evolution, a series of less severe bounces. Interestingly, although there are differences during the evolution between the various symmetries and topologies, the evolution on the other side of the bounce asymptotes to space-times of Nariai-type, with the exception of the planar black hole analyzed here, whose $T$-$R$=constant subspaces seem to continue expanding in the long term evolution. For the other cases, Nariai-type universes are attractors in the quantum evolution, albeit with different parameters. We study here the quantum evolution of each symmetry in detail.

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