Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
arXiv:1607.03928 · doi:10.1155/2016/7380372
Abstract
In this paper, we propose a new approach to study the dark sector of the universe by considering the dark energy as emerging a q-deformed bosonic scalar field which is not only interacting with the dark matter, but also non-minimally coupled to gravity, in the framework of standard Einsteinian gravity. In order to analyze the dynamic of the system, we first give the quantum field theoretical description of the q-deformed scalar field dark energy, then construct the action and the dynamical structure of these interacting and non-minimally coupled dark sector. As a second issue, we perform the phase space analysis of the model to check the reliability of our proposal by searching the stable attractor solutions implying the late-time accelerating expansion phase of the universe.
References in corpus (23)
- Dynamics of dark energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Cosmology and the Fate of Dilatation Symmetry
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Cosmological Evolution of a Quintom Model of Dark Energy
- Can dark energy evolve to the Phantom?
- Coupled oscillators as models of quintom dark energy
- Quintom cosmologies admitting either tracking or phantom attractors
- Quintom cosmologies with arbitrary potentials
- Two-Field Quintom Models in the w-w' Plane
- Crossing the Phantom Divide
- Quintom model with O() symmetry
- Constraints on the Sound Speed of Dynamical Dark Energy
- Holographic Foam, Dark Energy and Infinite Statistics
- Inflation by non-minimal coupling
- Extended Quintessence with non-minimally coupled phantom scalar field
- On the dynamics of a quadratic scalar field potential
- Generating Scale-Invariant Perturbations from Rapidly-Evolving Equation of State
- Non-minimally coupled scalar field cosmology on the phase plane
- Asymptotic behavior of w in general quintom model
- Attractors, Universality and Inflation
- Dynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space Analysis
- Deformed Quantum Field Theory, Thermodynamics at Low and High Energies, and Gravity. I