Qualitative dynamics and inflationary attractors in loop cosmology

TL;DR

This paper analyzes the qualitative dynamics of three loop quantum cosmology models, revealing common features like quantum bounce and inflationary attractors, and compares their behaviors across different inflationary potentials.

Contribution

It provides a detailed dynamical systems analysis of three loop quantum cosmology models, including the first detailed study of mLQC-II, highlighting their similarities and differences in inflationary scenarios.

Findings

All models exhibit non-singular inflation with super-inflation phases.

Universal features include quantum bounce and inflationary attractors.

Pre-bounce dynamics differ notably between mLQC-I and the other models.

Abstract

Qualitative dynamics of three different loop quantizations of spatially flat isotropic and homogeneous models is studied using effective spacetime description of the underlying quantum geometry. These include the standard loop quantum cosmology (LQC), its recently revived modification (referred to as mLQC-I), and another related modification of LQC (mLQC-II) whose dynamics is studied in detail for the first time. Various features of LQC, including quantum bounce and pre-inflationary dynamics, are found to be shared with the mLQC-I and mLQC-II models. We study universal properties of dynamics for chaotic inflation, fractional monodromy inflation, Starobinsky potential, non-minimal Higgs inflation, and an exponential potential. We find various critical points and study their stability, which reveal various qualitative similarities in the post-bounce phase for all these models. The pre-bounce qualitative dynamics of LQC and mLQC-II turns out to be very similar, but is strikingly different from that of mLQC-I. In the dynamical analysis, some of the fixed points turn out to be degenerate for which center manifold theory is used. For all these potentials, non-perturbative quantum gravitational effects always result in a non-singular inflationary scenario with a phase of super-inflation succeeded by the conventional inflation. We show the existence of inflationary attractors, and obtain scaling solutions in the case of the exponential potential. Since all of the models agree with general relativity at late times, our results are also of use in classical theory where qualitative dynamics of some of the potentials has not been studied earlier.