The arbitrariness of potentials in interacting quintessence models
arXiv:1811.03234 · doi:10.1103/PhysRevD.99.123520
Abstract
We study the interacting quintessence model with two different types of interaction by introducing a general parameterization of the quintessence potentials. The form of the quintessence potentials is arbitrary as the recent cosmological observations failed to constrain any particular form of the potentials. We explore the interacting quintessence models and investigate if an introduction of interaction between the dark sectors can constrain any particular form of the potential. Our findings reconfirm the arbitrariness of the quintessence potentials even for the interacting dark energy models. As a result, it is shown that the current observations are able to put an upper bound to the interaction parameter for both of the interactions we consider, although it is not possible to constrain the form of the potentials.
arXiv comment9 pages, 6 figures
References in corpus (62)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Planck 2015 results. XIII. Cosmological parameters
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Cosmological parameters from SDSS and WMAP
- Cosmological Imprint of an Energy Component with General Equation of State
- Extended Theories of Gravity
- Cosmological Constant - the Weight of the Vacuum
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The Case for a Positive Cosmological Lambda-term
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- A 2.4% Determination of the Local Value of the Hubble Constant
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- f(T) teleparallel gravity and cosmology
- Exponential potentials and cosmological scaling solutions
- Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
- KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
- Dark Energy after GW170817: dead ends and the road ahead
- Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
- Dark Energy after GW170817 and GRB170817A
- Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
- Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
- Quintessence: A Review
- Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- On the Cosmological Implications of the String Swampland
- A New Cosmological Model of Quintessence and Dark Matter
- Dynamical systems applied to cosmology: dark energy and modified gravity
- Gravitational Lensing Analysis of the Kilo Degree Survey
- Planck 2015 results. XIV. Dark energy and modified gravity
- Inflationary cosmology in modified gravity theories
- Breaking a Dark Degeneracy with Gravitational Waves
- The first and second data releases of the Kilo-Degree Survey
- Challenges to Self-Acceleration in Modified Gravity from Gravitational Waves and Large-Scale Structure
- Interactions in Scalar Field Cosmology
- Hydrodynamical N-body simulations of coupled dark energy cosmologies
- Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
- Dark coupling
- Generalized Assisted Inflation
- Coupled and Extended Quintessence: theoretical differences and structure formation
- A model independent approach to the dark energy equation of state
- The Paths of Quintessence
- Applications of scalar attractor solutions to Cosmology
- Calibration of weak-lensing shear in the Kilo-Degree Survey
- General Scalar Fields as Quintessence
- Parametrization of Quintessence and Its Potential
- Phase-space analysis of interacting phantom cosmology
- Dynamics of Interacting Quintessence Models: Observational Constraints
- Towards accurate cosmological predictions for rapidly oscillating scalar fields as dark matter
- Asymptotic behavior of the warm inflation scenario with viscous pressure
- Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn
- Quintessence in a quandary: prior dependence in dark energy models
- Cosmological solutions in multidimensional model with multiple exponential potential
- New tracker models of dark energy
- Tracking quintessence: a dynamical systems study
- New general parametrization of quintessence fields and its observational constraints
- New perturbative method for analytical solutions in single-field models of inflation
Cited by in corpus (9)
- Dynamical dark energy in the light of DESI 2024 data
- Interacting quintessence in light of Generalized Uncertainty Principle: Cosmological perturbations and dynamics
- Dynamical systems analysis of tachyon dark energy model from a new perspective
- Interacting dark sector: a dynamical system perspective
- The Nature of Dark Energy and Constraints on Its Hypothetical Constituents from Force Measurements
- I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
- Constructing Viable Interacting Dark Matter and Dark Energy Models: A Dynamical Systems Approach
- Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
- Generic autonomous system approach to interacting dark energy models