Primordial Universe with radiation and Bose-Einstein condensate
F. G. Alvarenga, L. G. Ferreira Filho, R. Fracalossi, R. C. Freitas,, S. V. B. Gon\c{c}alves, G. A. Monerat, G. Oliveira-Neto, E. V. Corr\^ea, Silva

TL;DR
This paper explores a quantum cosmological model of the early universe composed of radiation and Bose-Einstein condensate, analyzing classical and quantum behaviors, including singularity avoidance and bouncing solutions.
Contribution
It introduces a novel quantum cosmological model with BEC and radiation, deriving solutions to the Wheeler-DeWitt equation and demonstrating singularity-free behavior.
Findings
Classical scale factor exhibits bouncing or Big Crunch solutions.
Quantum analysis yields finite-norm wave packets.
Model avoids cosmological singularities.
Abstract
In this work we derive a scenario {in which} the early universe consists of {radiation fluid} and Bose-Einstein condensate. The possibility of gravitational self-interaction due to an attractive Bose-Einstein condensate is analyzed. The classical behavior of the scale factor of the universe is determined by a parameter associated with the Bose-Einstein fluid with bouncing or Big Crunch solutions. After we proceed to compute the finite-norm wave packet solutions to the Wheeler-DeWitt equation. The behavior of the scale factor is studied by applying the many-worlds interpretation of quantum mechanics. The quantum cosmological model is free from the singularities.
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