Cosmological perturbations and dynamical analysis for interacting quintessence
arXiv:1908.03657 · doi:10.1140/epjc/s10052-019-7418-8
Abstract
We present the dynamical analysis for interacting quintessence, considering linear cosmological perturbations. Matter perturbations improve the background analysis and viable critical points describing the transition of the three cosmological eras are found. The stability of those fixed points are similar to previous studies in the literature, for both coupled and uncoupled cases, leading to a late-time attractor.
arXiv comment8 pages, 1 figure, references added, version accepted for publication in EPJC
References in corpus (97)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- Cosmological Imprint of an Energy Component with General Equation of State
- 4D Gravity on a Brane in 5D Minkowski Space
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- A Model of Holographic Dark Energy
- Coupled Quintessence
- Exponential potentials and cosmological scaling solutions
- Accelerated expansion of the universe driven by tachyonic matter
- Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
- Entropy Bounds and Dark Energy
- Dark Energy
- Holographic dark energy and cosmic coincidence
- Transition of the dark energy equation of state in an interacting holographic dark energy model
- Interacting Quintessence
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Cosmology with tachyon field as dark energy
- Interacting quintessence solution to the coincidence problem
- Interacting Dark Matter and Dark Energy
- Dynamical systems applied to cosmology: dark energy and modified gravity
- The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
- Quintessence and Supergravity
- Nonminimal coupling and quintessence
- Tale of stable interacting dark energy, observational signatures, and the tension
- Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
- Vector Field Models of Inflation and Dark Energy
- Constraints on the interacting holographic dark energy model
- Holographic dark energy models: A comparison from the latest observational data
- What is needed of a tachyon if it is to be the dark energy?
- Thermodynamics of an accelerated expanding universe
- Coupled dark energy: Towards a general description of the dynamics
- Constraints on the sum of the neutrino masses in dynamical dark energy models with are tighter than those obtained in CDM
- The landscape, the swampland and the era of precision cosmology
- Inflation and late-time cosmic acceleration in non-minimal Maxwell- gravity and the generation of large-scale magnetic fields
- Coupled and Extended Quintessence: theoretical differences and structure formation
- Testing the Interaction between Dark Energy and Dark Matter with Planck Data
- Challenges for scaling cosmologies
- Thermodynamical description of the interaction between holographic dark energy and dark matter
- Applications of scalar attractor solutions to Cosmology
- Probing interaction and spatial curvature in the holographic dark energy model
- Cosmological Evolution of Interacting Phantom Energy with Dark Matter
- Growth of perturbations in dark matter coupled with quintessence
- Cosmology of Mass-Varying Neutrinos Driven by Quintessence: Theory and Observations
- Matter density perturbations in interacting quintessence models
- Phase-space analysis of interacting phantom cosmology
- Interacting Phantom Energy
- Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
- Quintessence models in Supergravity
- Supergravity, Dark Energy and the Fate of the Universe
- Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
- Evidence for interacting dark energy from BOSS
- A Field Theory Model for Dark Matter and Dark Energy in Interaction
- General analytic formulae for attractor solutions of scalar-field dark energy models and their multi-field generalizations
- Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
- Constraints on flat cosmologies with tracking Quintessence from Cosmic Microwave Background observations
- Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
- Holographic dark energy from minimal supergravity
- Ricci-Gauss-Bonnet holographic dark energy
- Revisit of the interacting holographic dark energy model after Planck 2015
- Dynamics of dark energy models and centre manifolds
- Dark energy, the electroweak vacua and collider phenomenology
- Sensitivity of the Cosmic Microwave Background Anisotropy to Initial Conditions in Quintessence Cosmology
- Cosmological structure formation with clustering quintessence
- Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos
- Cosmological phase space analysis of the F (X) - V (phi) scalar field and bouncing solutions
- Extended quintessence with an exponential coupling
- Metastable Dark Energy with Radioactive-like Decay
- Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn
- Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
- Fine Tuning in Quintessence Models with Exponential Potentials
- Coupled Quintessence and the Halo Mass Function
- Massive Photon and Dark Energy
- Dark energy, the colored anti-de Sitter vacuum, and LHC phenomenology
- Coupled dark energy: a dynamical analysis with complex scalar field
- Dynamical system analysis at background and perturbation levels: Quintessence in severe disadvantage comparing to CDM
- Quintessence with Yukawa Interaction
- Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
- Dynamical analysis for a vector-like dark energy
- A Model for Dark Energy decay
- Metastable dark energy
- The transition of equation of state of effective dark energy in the DGP model with bulk contents
- Clustering of quintessence on horizon scales and its imprint on HI intensity mapping
- Possible solution to the main cosmological constant problem
- Coupled tachyonic dark energy: a dynamical analysis
- Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off
- CMB and matter power spectra with non-linear dark-sector interactions
- Dynamical system analysis for DBI dark energy interacting with dark matter
- Reconsidering a higher-spin-field solution to the main cosmological constant problem
- Cosmological implications of the transition from the false vacuum to the true vacuum state
- Reconstruction of interaction rate in Holographic dark energy
- Quantum mechanical look at the radioactive-like decay of metastable dark energy
- Vector-field model with compensated cosmological constant and radiation-dominated FRW phase
- Constraining coupled quintessence with the 21cm signal
- Perturbations of the Lambda-CDM model in a dynamical systems perspective
- Instability in interacting dark sector: An appropriate Holographic Ricci dark energy model
- Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
Cited by in corpus (12)
- Cosmology in gravity: A unified dynamical system analysis at background and perturbation levels
- Background evolution and growth of structures in interacting dark energy through dynamical system analysis
- Observational constraints and predictions of the interacting dark sector with field-fluid mapping
- Cosmological perturbations in the interacting dark sector: Mapping fields and fluids
- Fractional dark energy
- A note on interacting holographic dark energy with a Hubble-scale cutoff
- Stability analysis of f(Q) gravity models using dynamical systems
- Cosmological Evolution of Two-Scalar fields Cosmology in the Jordan frame
- Constraints on interacting dark energy revisited: implications for the Hubble tension
- Asymptotic behavior of -fields Chiral Cosmology
- Scalar field evolution at background and perturbation levels for a broad class of potentials
- New tests of dark sector interactions from the full-shape galaxy power spectrum