paper

A comprehensive analysis of the compact phase space for Hu-Sawicki dark energy models including spatial curvature

arXiv:2208.15002 · doi:10.1103/PhysRevD.106.103533

Abstract

We present a comprehensive dynamical systems analysis of homogeneous and isotropic Friedmann-Laîmatre-Robertson-Walker cosmologies in the Hu-Sawicki dark energy model for the parameter choice . For a generic theory, we outline the procedures of compactification of the phase space, which in general is 4-dimensional. We also outline how, given an model, one can determine the coordinate of the phase space point that corresponds to the present day universe and the equation of a surface in the phase space that represents the CDM evolution history. Next, we apply these procedures to the Hu-Sawicki model under consideration. We identify some novel features of the phase space of the model such as the existence of invariant submanifolds and 2-dimensional sheets of fixed points. We determine the physically viable region of the phase space, the fixed point corresponding to possible matter dominated epochs and discuss the possibility of a non-singular bounce, re-collapse and cyclic evolution. We also provide a numerical analysis comparing the CDM evolution and the Hu-Sawicki evolution.

23 pages, 9 figures

References in corpus (13)

Cited by in corpus (3)