Bianchi type I, Schutz perfect fluid and evolutionary quantum cosmology
Fatimah Tavakoli, Babak Vakili

TL;DR
This paper explores classical and quantum cosmology of a Bianchi type I universe with a perfect fluid, using Schutz formalism to identify a time parameter, and investigates quantum effects that may prevent classical singularities.
Contribution
It introduces a novel application of Schutz formalism to Bianchi type I cosmology, deriving a Schrödinger-like WDW equation and analyzing singularity avoidance via quantum potential.
Findings
Classical universe expands from a big-bang singularity.
Quantum wave functions are constructed explicitly.
Quantum effects suggest possible singularity avoidance.
Abstract
We study the classical and quantum cosmology of a universe in which the matter content is a perfect fluid and the background geometry is described by a Bianchi type I metric. To write the Hamiltonian of the perfect fluid we use the Schutz representation, in terms of which, after a particular gauge fixing, we are led to an identification of a clock parameter which may play the role of time for the corresponding dynamical system. In view of the classical cosmology, it is shown that the evolution of the universe represents a late time expansion coming from a big-bang singularity. We also consider the issue of quantum cosmology in the framework of the canonical Wheeler-DeWitt (WDW) equation. It is shown that the Schutz formalism leads to the introduction of a momentum that enters linearly into Hamiltonian. This means that the WDW equation takes the form of a Schr\"{o}dinger equation for the…
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