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Loop quantization of the Schwarzschild black hole
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Loop quantization of the Schwarzschild black hole
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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.
Forward citations
Cited by 2 Pith papers
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Orbital Dynamics and Gravitational-Wave Signatures of EMRIs in Self-Dual Loop Quantum Gravity Black Holes
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.
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Quasinormal Modes of Self-Dual Loop Quantum Gravity Corrected Kerr Black Holes
In a rotating LQG-corrected black hole model, the polymeric parameter P lowers scalar quasinormal-mode frequencies, while spin raises them.
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