Quadratic quantum cosmology with Schutz' perfect fluid

TL;DR

This paper explores classical and quantum cosmological models with a perfect fluid in quadratic $f(R)$ gravity, deriving a Schrödinger-Wheeler-DeWitt equation and obtaining exact solutions for specific cases.

Contribution

It introduces a novel approach using Schutz' fluid representation to identify a time parameter and derives exact quantum solutions in quadratic $f(R)$ gravity.

Findings

Exact solutions to the SWD equation for $f(R)=R^2$ model.

Comparison of quadratic and linear $f(R)$ models.

Identification of a time parameter in quantum cosmology.

Abstract

We study the classical and quantum models of a Friedmann-Robertson-Walker (FRW) cosmology, coupled to a perfect fluid, in the context of the $f(R)$ gravity. Using the Schutz' representation for the perfect fluid, we show that, under a particular gauge choice, it may lead to the identification of a time-parameter for the corresponding dynamical system. Moreover, this formalism gives rise to a Schr\"{o}dinger-Wheeler-DeWitt (SWD) equation for the quantum-mechanical description of the model under consideration, the eigenfunctions of which can be used to construct the wavefunction of the Universe. In the case of $f(R)=R^2$ (pure quadratic model), for some particular choices of the perfect fluid source, exact solutions to the SWD equation can be obtained and the corresponding results are compared to the usual $f(R)=R$ model.