Quantum cosmological perfect fluid model and its classical analogue
A.B. Batista, J.C. Fabris, S.V.B. Goncalves, Joel Tossa, (Departamento de Fisica, Universidade Federal do Espirito Santo, Brazil)

TL;DR
This paper explores quantum cosmology with perfect fluids, showing that quantum effects lead to a bouncing universe and that these models have a universal classical analogue involving a repulsive stiff matter fluid.
Contribution
It demonstrates the quantum behavior of perfect fluid cosmological models and establishes their universal classical analogue with a repulsive stiff matter component.
Findings
Quantum models predict a bouncing, non-singular universe.
Quantum scenarios are equivalent to classical models with a repulsive stiff matter fluid.
Flat and non-flat cases are mathematically equivalent to free particles and harmonic oscillators, respectively.
Abstract
The quantization of gravity coupled to a perfect fluid model leads to a Schr\"odinger-like equation, where the matter variable plays the role of time. The wave function can be determined, in the flat case, for an arbitrary barotropic equation of state ; solutions can also be found for the radiative non-flat case. The wave packets are constructed, from which the expectation value for the scale factor is determined. The quantum scenarios reveal a bouncing Universe, free from singularity. We show that such quantum cosmological perfect fluid models admit a universal classical analogue, represented by the addition, to the ordinary classical model, of a repulsive stiff matter fluid. The meaning of the existence of this universal classical analogue is discussed. The quantum cosmological perfect fluid model is, for a flat spatial section, formally equivalent to a free particle…
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