Quantum gravitational onset of Starobinsky inflation in a closed universe

TL;DR

This paper demonstrates that quantum gravity effects in loop quantum cosmology enable the successful onset of low energy scale Starobinsky inflation in a closed universe, overcoming classical recollapse and singularity issues.

Contribution

It shows that quantum gravitational cyclic evolution allows low energy inflation to start in closed universes, which is impossible in classical theory.

Findings

Quantum gravity resolves big crunch singularities.

Starobinsky inflation can begin from various initial conditions.

Pre-inflationary cycles facilitate suitable conditions for inflation.

Abstract

Recent cosmic microwave background observations favor low energy scale inflationary models in a closed universe. However, onset of inflation in such models for a closed universe is known to be severely problematic. In particular, such a universe recollapses within a few Planck seconds and encounters a big crunch singularity when initial conditions are given in the Planck regime. We show that this problem of onset of inflation in low energy scale inflationary models can be successfully overcome in a quantum gravitational framework where the big bang/big crunch singularities are resolved and a non-singular cyclic evolution exists prior to inflation. As an example we consider a model in loop quantum cosmology and demonstrate that the successful onset of low energy scale inflation in a closed universe is possible for the Starobinsky inflationary model starting from a variety of initial conditions where it is impossible in the classical theory. For comparison we also investigate the onset of inflation in the $\phi^2$ inflationary model under similar unfavorable conditions. The pre-inflationary phase with quantum gravity effects is shown to be composed of non-identical cycles of bounces and recollapses resulting in a hysteresis-like phenomenon, which plays an important role in creating suitable conditions for inflation to occur after some number of non-singular cycles. Our analysis shows that the tension in the classical theory amounting to the unsuitability of closed FLRW universes with respect to the onset of low energy scale inflation can be successfully resolved in loop quantum cosmology.