Derives loop-quantum-corrected effective dynamics for spherical symmetry via path integral, yielding a black hole geometry with curvature singularity but no null geodesic incompleteness.
Tibrewala, Spherically symmetric einstein maxwell theory and loop quantum gravity corrections, Classical and Quantum Gravity 29, 235012 (2012)
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Effective spherical symmetry in Loop Quantum Gravity: A path integral approach
Derives loop-quantum-corrected effective dynamics for spherical symmetry via path integral, yielding a black hole geometry with curvature singularity but no null geodesic incompleteness.