Loop quantum black hole

Abstract

In the last decades, progress on the quantization of black holes using techniques developed in loop quantum cosmology has received increasing attention. Due to the quantum geometry effect, the resulting quantum corrected black hole is free of singularity. The quantization scheme can be roughly divided into four types, that is 1. ${\mu }_0$-scheme, 2. $\bar{\mu }$-scheme, 3. generalized ${\mu }_0$-scheme, 4. quantum collapsing model. This paper provides an introduction of the loop quantum black hole models and a summary of the progress made in this field, as well as the quantum effective dynamics and physical applications of these models.

arXiv commentA mini review, 15 pages

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Cited by in corpus (18)

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• Status of Birkhoff's theorem in polymerized semiclassical regime of Loop Quantum Gravity
• Effective four-dimensional loop quantum black hole with a cosmological constant
• The Lensing Effect of Quantum-Corrected Black Hole and Parameter Constraints from EHT Observations
• Higher-dimensional quantum Oppenheimer-Snyder model
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• Quasinormal modes of a nonsingular spherically symmetric black hole effective model with holonomy corrections
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• Image of a quantum-corrected black hole without Cauchy horizons illuminated by a static thin accretion disk
• Critical collapse of a massive scalar field in semi-classical loop quantum gravity
• Higher-dimensional quantum-corrected Oppenheimer-Snyder model with a cosmological constant