The past and future dynamics of quintom dark energy models
arXiv:1808.05634 · doi:10.1140/epjc/s10052-018-6225-y
Abstract
We study the phase space of the quintom cosmologies for a class of exponential potentials. We combine normal forms expansions and the center manifold theory in order to describe the dynamics near equilibrium sets. Furthermore, we construct the unstable and center manifold of the massless scalar field cosmology motivated by the numerical results given in Lazkoz and Leon (Phys Lett B 638:303. arXiv:astro-ph/0602590, 2006). We study the role of the curvature on the dynamics. Several monotonic functions are defined on relevant invariant sets for the quintom cosmology. Finally, conservation laws of the cosmological field equations and algebraic solutions are determined by using the symmetry analysis and the singularity analysis.
22 pages, 3 compound figures (13 eps files)
References in corpus (33)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Cosmological Evolution of a Quintom Model of Dark Energy
- Reconstructing Dark Energy
- Towards a Nonsingular Bouncing Cosmology
- Bouncing Universe with Quintom Matter
- Cosmological Solutions of Gravity
- Generalized Second Law of Thermodynamics in Quintom Dominated Universe
- Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
- Inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills- gravity and non-minimal vector- gravity
- Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
- Coupled oscillators as models of quintom dark energy
- Quintom cosmologies admitting either tracking or phantom attractors
- Using the Noether symmetry approach to probe the nature of dark energy
- Quintom cosmologies with arbitrary potentials
- A String-Inspired Quintom Model Of Dark Energy
- Dark Energy Model with Spinor Matter and Its Quintom Scenario
- Unified dark energy thermodynamics: varying w and the -1-crossing
- Late acceleration and crossing in induced gravity
- Transition from quintessence to phantom phase in quintom model
- Braneworld models with a non-minimally coupled phantom bulk field: a simple way to obtain the -1-crossing at late times
- Two scalar field cosmology: Conservation laws and exact solutions
- Invariant solutions and Noether symmetries in Hybrid Gravity
- Noether analysis of Scalar-Tensor Cosmology
- Reconstructing a String-Inspired Quintom Model of Dark Energy
- The w = -1 crossing of the quintom model with slowly-varying potentials
- Theoretical Aspects of Quintom Models
- Analytical solutions in cosmology from singularity analysis
- Analytic Solution of the Starobinsky Model for Inflation
- Asymptotic behavior of w in general quintom model
- Higher Order Lagrangians inspired by the Pais-Uhlenbeck Oscillator and their cosmological applications
Cited by in corpus (49)
- In the Realm of the Hubble tension a Review of Solutions
- Cosmological solutions and growth index of matter perturbations in gravity
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Selected topics in scalar-tensor theories and beyond
- Dark energy in light of the early JWST observations: case for a negative cosmological constant?
- Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
- Dynamics of nonlinear interacting dark energy models
- Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
- Dynamics of a two scalar field cosmological model with phantom terms
- Exact Solutions in Chiral Cosmology
- Bayesian evidence for -attractor dark energy models
- Extended phase-space analysis of the Horava-Lifshitz cosmology
- Dynamics of Einstein-Aether Scalar field Cosmology
- Complete cosmological model based on a asymmetric scalar Higgs doublet
- The Oscillatory Universe, phantom crossing and the Hubble tension
- Cosmological Evolution of Two-Scalar fields Cosmology in the Jordan frame
- Integrable modified gravity cosmological models with an additional scalar field
- Classical and quantum exact solutions for a FRW in chiral like cosmology
- Cosmological Models Based on a Statistical System of Scalar Charged Degenerate Fermions and an Asymmetric Higgs Scalar Doublet
- Generalized scalar field cosmologies: theorems on asymptotic behavior
- Stability of a modified Jordan-Brans-Dicke theory in the dilatonic frame
- Time-averaging axion-like interacting scalar fields models
- Conservation laws and Exact Solutions in Brans-Dicke Cosmology with a Scalar Field
- Generalized Scalar Field Cosmologies: A Global Dynamical Systems Formulation
- Averaging Generalized Scalar Field Cosmologies I: Locally Rotationally Symmetric Bianchi III and open Friedmann-Lemaître-Robertson-Walker models
- Multi-fluid cosmology in Einstein gravity: analytical solutions
- Dynamical description of a quintom cosmological model nonminimally coupled with gravity
- Extended analysis for the Evolution of the Cosmological history in Einstein-aether Scalar Field theory
- Quintom fields from chiral K-essence cosmology
- Early dark energy and the screening mechanism
- Analytic solutions in Einstein-aether scalar field cosmology
- Fractional Einstein-Gauss-Bonnet scalar field cosmology
- Asymptotic behavior of -fields Chiral Cosmology
- Similarity of cosmological models and its application to the analysis of cosmological evolution
- Cosmological Boundary Flux Parameter
- Cosmological evolution of a statistical system of degenerate scalar-charged fermions with an asymmetric scalar doublet. I. Two-component system of assorted charges
- Scalar field evolution at background and perturbation levels for a broad class of potentials
- Stability analysis of an interacting holographic dark energy model
- Anisotropic chiral cosmology: exact solutions
- Quintessence scalar field and cosmological constant: Dynamics of a multi-component dark energy model
- Modified Brans-Dicke cosmology with Minimum Length Uncertainty
- From inflation to dark energy in scalar-tensor cosmology
- The sounds of science a symphony for many instruments and voices part II
- Early dark energy and scalarization in a scalar-tensor model
- Self-gravitating Higgs field of scalar charge. II. Asymmetric scalar doublet
- Revisiting cosmological diffusion models in Unimodular Gravity and the tension
- Correlation of structure growth index with current cosmic acceleration: constraints on dark energy models
- Cosmological models based on an asymmetric scalar doublet with kinetic coupling of components. I. General properties of the cosmological model
- Evolution of matter perturbations in the context of cosmic slowing down