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Spherically Symmetric Quantum Geometry: Hamiltonian Constraint

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arxiv gr-qc/0511108 v1 pith:NHGV2AEP submitted 2005-11-18 gr-qc

Spherically Symmetric Quantum Geometry: Hamiltonian Constraint

classification gr-qc
keywords symmetricsphericallyfurthermodelsquantumhamiltonianschemeadapted
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Variables adapted to the quantum dynamics of spherically symmetric models are introduced, which further simplify the spherically symmetric volume operator and allow an explicit computation of all matrix elements of the Euclidean and Lorentzian Hamiltonian constraints. The construction fits completely into the general scheme available in loop quantum gravity for the quantization of the full theory as well as symmetric models. This then presents a further consistency check of the whole scheme in inhomogeneous situations, lending further credence to the physical results obtained so far mainly in homogeneous models. New applications in particular of the spherically symmetric model in the context of black hole physics are discussed.

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Cited by 4 Pith papers

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

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  2. Quasinormal modes of a rotating loop quantum black hole

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    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.

  4. 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.