Cosmological dynamics of a hybrid chameleon scenario
Kourosh Nozari, N. Rashidi

TL;DR
This paper investigates a hybrid chameleon cosmological model with a non-minimally coupled scalar field, analyzing its stability, phase space, and the universe's evolution, including phantom divide crossing.
Contribution
It introduces a hybrid chameleon model with an effective potential, analyzing its phase space and stability, and demonstrates the universe's evolution features within this framework.
Findings
Hybrid chameleon domination is a stable attractor.
The universe experiences phantom divide crossing.
Effective potential depends on local matter density.
Abstract
We consider a hybrid scalar field which is non-minimally coupled to the matter and models a chameleon cosmology. By introducing an effective potential, we study the dependence of the effective potential's minimum and hybrid chameleon field's masses to the local matter density. In a dynamical system technique, we analyze the phase space of this two-field chameleon model, find its fixed points and study their stability. We show that the hybrid chameleon domination solution is a stable attractor and the universe in this setup experiences a phantom divide crossing.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena
