Quantum cosmology of a Bianchi III LRS geometry coupled to a source free electromagnetic field
A. Karagiorgos, T. Pailas, N. Dimakis, Petros A. Terzis, T., Christodoulakis

TL;DR
This paper explores the classical and quantum properties of a Bianchi III LRS cosmological model coupled with an electromagnetic field, revealing a connection to black hole solutions and producing singularity-free semi-classical geometries.
Contribution
It introduces a novel analysis of Bianchi III LRS cosmology with electromagnetic fields, linking classical solutions to black hole metrics and deriving quantum wave functions with singularity avoidance.
Findings
Classical solutions include time-dependent electric and constant magnetic charges.
The mini-superspace resembles the Reissner-Nordström black hole metric.
Quantum states lead to semi-classical, mostly singularity-free geometries.
Abstract
We consider a Bianchi type III axisymmetric geometry in the presence of an electromagnetic field. A first result at the classical level is that the symmetry of the geometry need not be applied on the electromagnetic tensor ; the algebraic restrictions, implied by the Einstein field equations to the stress energy tensor , suffice to reduce the general to the appropriate form. The classical solution thus found contains a time dependent electric and a constant magnetic charge. The solution is also reachable from the corresponding mini-superspace action, which is strikingly similar to the Reissner-Nordstr{\"o}m one. This points to a connection between the black hole geometry and the cosmological solution here found, which is the analog of the known correlation between the Schwarzschild and the Kantowski-Sachs metrics. The configuration space is…
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