Relational quantum dynamics of the black hole interior: singularity resolution and quantum bounce
Paolo Fragolino, Saeed Rastgoo

TL;DR
This paper presents a relational, gauge-invariant quantum analysis of black hole interiors, demonstrating singularity resolution and a quantum bounce that suggests a transition from black hole to white hole.
Contribution
It introduces a fully relational and gauge-invariant quantization framework for black hole interiors, showing singularity resolution and a quantum bounce without relying on specific quantization schemes.
Findings
Kretschmann and expansion scalars remain finite inside the black hole.
The area of 2-spheres is bounded below by a minimum value.
The expansion scalar vanishes and changes sign at the quantum bounce.
Abstract
We study the interior of the Schwarzschild black hole which is isometric to the Kantowski-Sachs cosmological model, using a fully relational and gauge-invariant quantization framework. The physical Hilbert space is constructed via refined algebraic quantization, and quantum dynamics is recovered through the Page-Wootters formalism with a covariant POVM clock built from one of the two configuration variables, whose Hamiltonian is proportional to the momentum of the said variable. Gauge-invariant relational observables for the area of 2-spheres, the Kretschmann scalar, and the expansion scalar of null geodesic are constructed via group averaging (G-twirl) and evaluated on physical states. We find that the Kretschmann and expansion scalars remain finite throughout the black hole, while the area of 2-spheres is bounded below by a minimum value proportional to the uncertainty in the system…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
