The Born-Oppenheimer approach to Quantum Cosmology

TL;DR

This paper compares two Born-Oppenheimer approaches to solving the Wheeler-DeWitt equation in quantum cosmology, analyzing their consistency and deriving perturbation equations for a flat inflaton potential.

Contribution

It introduces and compares a generalized BO decomposition with the standard approach, assessing their consistency and applicability in quantum cosmology models.

Findings

The generalized BO decomposition is consistent with the standard approach.

Derived Mukhanov-Sasaki equations for different decompositions.

Presented solutions to the homogeneous Wheeler-DeWitt equation beyond traditional BO methods.

Abstract

The scope of this paper is to compare two different approaches for solving the Wheeler-DeWitt (WDW) equation in the presence of homogeneous matter (inflaton) and perturbations around it. The standard Born-Oppenheimer (BO) decomposition, which consists of factorizing out the gravitational wave function and then defining the flow of the time through it, and a more general BO decomposition where the whole minisuperspace wave function is factorized out. The two approaches are compared, for simplicity, in the case of a minimally coupled inflaton with a flat potential. The consistency of the latter decomposition is checked against the former by comparing the resulting perturbation (Mukhanov-Sasaki) equations. Finally a few solutions to the homogeneous WDW not suitable for the traditional BO treatment are presented and the corresponding Mukhanov-Sasaki equations are evaluated.