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Loop quantization of the Schwarzschild black hole

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arxiv 1302.5265 v2 pith:XVZKV5Z3 submitted 2013-02-21 gr-qc hep-thquant-ph

Loop quantization of the Schwarzschild black hole

classification gr-qc hep-thquant-ph
keywords quantumalgebragravityloopblackclassicalconstraintconstraints
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We quantize spherically symmetric vacuum gravity without gauge fixing the diffeomorphism constraint. Through a rescaling, we make the algebra of Hamiltonian constraints Abelian and therefore the constraint algebra is a true Lie algebra. This allows the completion of the Dirac quantization procedure using loop quantum gravity techniques. We can construct explicitly the exact solutions of the physical Hilbert space annihilated by all constraints. New observables living in the bulk appear at the quantum level (analogous to spin in quantum mechanics) that are not present at the classical level and are associated with the discrete nature of the spin network states of loop quantum gravity. The resulting quantum space-times resolve the singularity present in the classical theory inside black holes.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Orbital Dynamics and Gravitational-Wave Signatures of EMRIs in Self-Dual Loop Quantum Gravity Black Holes

    gr-qc 2026-07 reject novelty 4.0

    The paper computes EMRI orbits and waveforms in self-dual LQG black hole spacetimes and claims Fisher-matrix constraints on the quantum parameters P and a0, but the Fisher forecast uses the metric itself as the observable.

  2. Quasinormal Modes of Self-Dual Loop Quantum Gravity Corrected Kerr Black Holes

    gr-qc 2026-07 reject novelty 2.0

    In a rotating LQG-corrected black hole model, the polymeric parameter P lowers scalar quasinormal-mode frequencies, while spin raises them.