Holographic kinetic k-essence model

Abstract

We consider a connection between the holographic dark energy density and the kinetic k-essence energy density in a flat FRW universe. With the choice $c\ge 1$, the holographic dark energy can be described by a kinetic k-essence scalar field in a certain way. In this paper we show this kinetic k-essential description of the holographic dark energy with $c\ge 1$ and reconstruct the kinetic k-essence function F(X).

6 pages, 4 figures, revised version, accepted for publication in Phys.Lett.B

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
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• The World as a Hologram
• Cosmological parameters from SDSS and WMAP
• 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
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• Phantom Energy and Cosmic Doomsday
• The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• A Model of Holographic Dark Energy
• Essentials of k-essence
• Cosmological Results from High-z Supernovae
• Cosmological Tracking Solutions
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Dark Energy Constraints from the Cosmic Age and Supernova
• Rolling Tachyon
• Tachyon Matter
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
• Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Entropy Bounds and Dark Energy
• The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
• Cosmological Evolution of a Quintom Model of Dark Energy
• The large-scale structure of the Universe
• CDM Models with a Smooth Component
• A classification of scalar field potentials with cosmological scaling solutions
• Purely kinetic k-essence as unified dark matter
• Constraints on holographic dark energy from type Ia supernova observations
• Dark Energy: Vacuum Fluctuations, the Effective Phantom Phase, and Holography
• A correlation of the cosmic microwave sky with large scale structure
• Hessence: A New View of Quintom Dark Energy
• Holographic Chaplygin gas model
• Supernova Constraints on a holographic dark energy model
• Tracking K-essence
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Reconstructing holographic quintessence
• Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
• Constraints on the Dark Energy from the holographic connection to the small l CMB Suppression
• Holographic tachyon model of dark energy
• Kinetic k-essence and Quintessence
• Joint CMB and Weak Lensing Analysis; Physically Motivated Constraints on Cosmological Parameters
• Holographic tachyon model
• Searching for a holographic connection between dark energy and the low-l CMB multipoles
• Crossing $w=-1$ by a single scalar on a Dvali-Gabadadze-Porrati brane
• Critical comments on the paper "Crossing $\omega =-1$ by a single scalar field on a Dvali-Gabadadze-Porrati brane" by H Zhang and Z-H Zhu [Phys.Rev.D75,023510(2007)]
• Cosmographic evaluation of deceleration parameter using SNe Ia data
• CMB Constraints on the Holographic Dark Energy Model
• A Detection of the Integrated Sachs-Wolfe Effect
• Reconstructing K-essence
• Investigating the origins of the CMB-XRB cross correlation
• Dark energy without dark energy
• Accelerating Hilbert-Einstein universe without dynamic dark energy
• Quantum cosmic models and thermodynamics

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• An equation of state for purely kinetic k-essence inspired by cosmic topological defects
• Evaluation of cosmological models in $f(R,T)$ gravity in different dark energy scenario
• Compatibility between the scalar field models of tachyon, $k$-essence and quintessence in $f(R,T)$ gravity
• Self-interacting holographic dark energy
• Crossing the phantom divide line in the Holographic dark energy model in a closed universe
• K-essence and kinetic gravity braiding models in two-field measure theory
• Cosmological constraints on a unified dark matter-energy scalar field model with fast transition
• Holographic dilatonic model of dark energy
• Holographic reconstruction of the k-essence and dilaton models
• Polytropic gas scalar field models of dark energy
• Thawing k-essence dark energy in the PAge space
• NEC violation in $f(\bar{R},\bar{T})$ gravity in the context of a non-canonical theory via modified Raychaudhuri equation
• Geometric sigma model of the Universe