Slow-roll k-essence
arXiv:0906.0628 · doi:10.1103/PhysRevD.80.043517
Abstract
We derive slow-roll conditions for thawing k-essence with a separable Lagrangian . We examine the evolution of the equation of state parameter, , as a function of the scale factor , for the case where is close to -1. We find two distinct cases, corresponding to and , respectively. For the case where the evolution of and hence is described by only two parameters, and is model-independent and coincides with similar behavior seen in thawing quintessence models. This result also extends to non-separable Lagrangians where . For the case , an expression is derived for , but this expression depends on the potential , so there is no model-independent limiting behavior. For the case, we derive observational constraints on the two parameters of the model, (the present-day value of ), and the , which parametrizes the curvature of the potential. We find that the observations sharply constrain to be close to -1, but provide very poor constraints on .
7 pages and 5 figures, typos corrected
References in corpus (35)
- Dynamics of dark energy
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Cosmological Imprint of an Energy Component with General Equation of State
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- k-Inflation
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Cosmological Tracking Solutions
- Kinetically Driven Quintessence
- Can the dark energy equation-of-state parameter w be less than -1?
- Rolling Tachyon
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
- The phantom menaced: constraints on low-energy effective ghosts
- Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes
- A classification of scalar field potentials with cosmological scaling solutions
- Tracking K-essence
- The Effective Theory of Quintessence: the w<-1 Side Unveiled
- Thawing quintessence with a nearly flat potential
- The Paths of Quintessence
- Dark energy from a quintessence (phantom) field rolling near potential minimum (maximum)
- Hilltop Quintessence
- DBI-essence
- Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
- Slow-Roll Thawing Quintessence
- Phantom Dark Energy Models with a Nearly Flat Potential
- The null energy condition and instability
- Instabilities and the null energy condition
- Measuring deviations from a cosmological constant: a field-space parameterization
- Dark Energy from a Phantom Field Near a Local Potential Minimum
- The transient and the late time attractor tachyon dark energy: Can we distinguish it from quintessence ?
- Bright High z SnIa: A Challenge for LCDM?
- Dark radiation as a signature of dark energy
Cited by in corpus (54)
- Cosmology and Fundamental Physics with the Euclid Satellite
- Cosmology and fundamental physics with the Euclid satellite
- Quintessence: A Review
- f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis
- Observational Constraints on Quintessence: Thawing, Tracker, and Scaling models
- Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?
- Designing a space-based galaxy redshift survey to probe dark energy
- Pure kinetic k-essence as the cosmic speed-up
- Dark Energy in Practice
- On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
- How clustering dark energy affects matter perturbations
- Quintessence and phantoms in light of DESI 2025
- Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
- Updated observational constraints on quintessence dark energy models
- Cosmological Dynamics of a Dirac-Born-Infeld field
- Phase-space analysis of a class of k-essence cosmology
- Constraints on a CDM model from strong gravitational lensing and updated Hubble parameter measurements
- Testing for dynamical dark energy models with redshift-space distortions
- Dark energy reconstruction based on the PADE approximation; an expansion around the CDM
- Recent advances in cosmological singularities
- Evaluation of cosmological models in gravity in different dark energy scenario
- Distance Measurements from Supernovae and Dark Energy Constraints
- Approximation of the potential in scalar field dark energy models
- Observational constraints on Horava-Lifshitz cosmology
- The Equation of State of Tracker Fields
- Does CDM really be in tension with the Hubble diagram data?
- A one-parameter formula for testing slow-roll dark energy: observational prospects
- Horava-Lifshitz cosmology with generalized Chaplygin gas
- Compatibility between the scalar field models of tachyon, -essence and quintessence in gravity
- Geometrical diagnostic for purely kinetic k-essence dark energy
- Quantum fractionary cosmology: K-essence theory
- The general property of dynamical quintessence field
- Using newest VLT-KMOS HII Galaxies and other cosmic tracers to test the CDM tension
- Overall observational constraints on the running parameter λof Horava-Lifshitz gravity
- Growth of perturbations in dark energy parametrization scenarios
- On the effect of the degeneracy between w_0 and w_a
- Constraining cosmologies with fundamental constants I. Quintessence and K-Essence
- Slow-roll Extended Quintessence
- Type V singularities in non-standard cosmological backgrounds
- Parametrization for the Scale Dependent Growth in Modified Gravity
- Cosmological Coincidence without Fine Tuning
- Generalizing thawing dark energy models: the standard vis-à-vis model independent diagnostics
- Dissipative quintessence, and its cosmological implications
- Restrictions on purely kinetic k-essence
- Non-parametric modeling of the cosmological data, base on the distribution
- CMB power spectrum in the emergent universe with k-essence
- A new generic evolution for -essence dark energy with
- Thawing k-essence dark energy in the PAge space
- Statistics of Thawing K-essence Dark Energy Models
- Type V singularities with inhomogeneous equations of state
- Dark energy with : Asymptotic versus pseudo-
- Quark-Novae Ia in the Hubble diagram: Implications For Dark Energy
- A Jacobian generalization of the pseudo Nambu-Goldstone bosons potential
- Dark Energy, with Signatures