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Probing Loop Quantum Gravity with Evaporating Black Holes

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arxiv 1109.4239 v2 pith:7EOMYDLR submitted 2011-09-20 gr-qc astro-ph.COhep-phhep-th

Aurelien Barrau , Xiangyu Cao , Jacobo Diaz-Polo , Julien Grain , Thomas Cailleteau This is my paper
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keywords blackevaporatinggravityholesquantumloopaimsallow
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This letter aims at showing that the observation of evaporating black holes should allow distinguishing between the usual Hawking behavior and Loop Quantum Gravity (LQG) expectations. We present a full Monte-Carlo simulation of the evaporation in LQG and statistical tests that discriminate between competing models. We conclude that contrarily to what was commonly thought, the discreteness of the area in LQG leads to characteristic features that qualify evaporating black holes as objects that could reveal quantum gravity footprints.

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  1. Polymer Black Hole Surrounded by Quintessence

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    A polymer black hole with quintessence yields a shadow that can match Sgr A* for many combinations of free parameters while cooling and dimming the black hole.

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