Mass and Horizon Dirac Observables in Effective Models of Quantum Black-to-White Hole Transition
Norbert Bodendorfer, Fabio M. Mele, Johannes M\"unch

TL;DR
This paper explores the role of mass and horizon Dirac observables in effective loop quantum gravity models of black-to-white hole transitions, revealing new models and relations between observables and quantum effects.
Contribution
It introduces a new polymerization model that overcomes previous initial condition restrictions and clarifies the role of Dirac observables in quantum black hole models.
Findings
Existence of two relevant Dirac observables linked to black and white hole masses.
A new polymerization model allows for broader initial conditions.
Quantum effects impose a universal curvature bound, independent of mass relations.
Abstract
In the past years, black holes and the fate of their singularity have been heavily studied within loop quantum gravity. Effective spacetime descriptions incorporating quantum geometry corrections are provided by the so-called polymer models. Despite the technical differences, the main common feature shared by these models is that the classical singularity is resolved by a black-to-white hole transition. In a recent paper, we discussed the existence of two Dirac observables in the effective quantum theory respectively corresponding to the black and white hole mass. Physical requirements about the onset of quantum effects then fix the relation between these observables after the bounce, which in turn corresponds to a restriction on the admissible initial conditions for the model. In the present paper, we discuss in detail the role of such observables in black hole polymer models. First,…
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