Smooth Quantum Dynamics of Mixmaster Universe
Herv\'e Bergeron, Ewa Czuchry, Jean Pierre Gazeau, Przemys{\l}aw, Ma{\l}kiewicz, W{\l}odzimierz Piechocki

TL;DR
This paper develops a quantum model of the Mixmaster universe using affine coherent states, resolving classical singularities and revealing stable quantum states with implications for early universe cosmology.
Contribution
It introduces a novel quantum approach combining affine coherent states and adiabatic approximation to analyze the Mixmaster universe.
Findings
Classical singularity is resolved by a repulsive potential.
Quantum oscillations produce a radiation energy density term.
Lowest energy eigenstates are dynamically stable.
Abstract
We present a quantum version of the vacuum Bianchi IX model by implementing affine coherent state quantization combined with a Born-Oppenheimer-like adiabatic approximation. The analytical treatment is carried out on both quantum and semiclassical levels. The resolution of the classical singularity occurs by means of a repulsive potential generated by our quantization procedure. The quantization of the oscillatory degrees of freedom produces a radiation energy density term in the semiclassical constraint equation. The Friedmann-like lowest energy eigenstates of the system are found to be dynamically stable.
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