Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology

Abstract

In this work, we studied the Power Law and the Logarithmic Entropy Corrected versions of the Ricci Dark Energy (RDE) model in a spatially non-flat universe and in the framework of Hořava-Lifshitz cosmology. For the two cases containing non-interacting and interacting RDE and Dark Matter (DM), we obtained the exact differential equation that determines the evolutionary form of the RDE energy density parameter. Moreover, we obtained the expressions of the deceleration parameter $q$ and, using a parametrization of the equation of state (EoS) parameter ${\omega }_D$ as ${\omega }_D\left(z\right)={\omega }_0+{\omega }_{1}z$, we derived the expressions of both ${\omega }_0$ and ${\omega }_1$. We interestingly found that the expression of ${\omega }_0$ is the same for both non-interacting and interacting case. The expression of ${\omega }_1$ for the interacting case has strong dependence from the interacting parameter $b^2$. The parameters derived in this work are done in small redshift approximation and for low redshift expansion of the EoS parameter.

arXiv admin note: text overlap with arXiv:1101.1774 by other authors

References in corpus (66)

• Dynamics of dark energy
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Quantum Gravity at a Lifshitz Point
• Cosmology and the Fate of Dilatation Symmetry
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Observational Signatures and Non-Gaussianities of General Single Field Inflation
• Spectral Dimension of the Universe in Quantum Gravity at a Lifshitz Point
• Cosmological Evolution of a Quintom Model of Dark Energy
• Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
• Membranes at Quantum Criticality
• A Holographic Dark Energy Model from Ricci Scalar Curvature
• Horava-Lifshitz Cosmology
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• Horava-Lifshitz Cosmology: A Review
• Chiral Primordial Gravitational Waves from a Lifshitz Point
• Lorentz symmetry breaking as a quantum field theory regulator
• Cosmology of the Lifshitz universe
• Black holes in asymptotically Lifshitz spacetime
• FRW Cosmology in F(R,T) gravity
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• Statefinder Diagnosis for Ricci Dark Energy
• Holographic dark energy with varying gravitational constant
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• Restoring Holographic Dark Energy in Brane Cosmology
• A Trouble with Hořava-Lifshitz Gravity
• Coupled oscillators as models of quintom dark energy
• Interacting models may be key to solve the cosmic coincidence problem
• Correspondence between Holographic and Gauss-Bonnet dark energy models
• Power-law corrections to entanglement entropy of horizons
• Observational constraints on the dark energy and dark matter mutual coupling
• The role of exterior Weyl fluids on compact stellar structures in Randall-Sundrum gravity
• Quintom model with O($N$) symmetry
• Viscous Ricci Dark Energy
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
• The generalized second law of thermodynamics in Horava-Lifshitz cosmology
• Entropy-Corrected Holographic Dark Energy
• Multifield DBI Inflation and Non-Gaussianities
• New agegraphic dark energy in Horava-Lifshitz cosmology
• Unifying inflation with dark energy in modified F(R) Horava-Lifshitz gravity
• An Alternative Approach for General Covariant Horava-Lifshitz Gravity and Matter Coupling
• Primordial perturbation with a modified dispersion relation
• Constraints on coupling constant between dark energy and dark matter
• The Effect of a Chameleon Scalar Field on the Cosmic Microwave Background
• Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models
• Reconstructing Quintom from Ricci Dark Energy
• A model of interacting holographic dark energy at the Ricci's scale
• Interacting entropy-corrected agegraphic-tachyon dark energy
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• 2-loop Quantum Yang-Mills Condensate as Dark Energy
• Stability of spin-0 graviton and strong coupling in Horava-Lifshitz theory of gravity
• Origin of holographic dark energy models
• Yang-Mills condensate dark energy coupled with matter and radiation
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Processing of Cosmological Perturbations in a Cyclic Cosmology
• Reconstructing $f(R)$ Theory from Ricci Dark Energy
• z=3 Lifshitz-Horava model and Fermi-point scenario of emergent gravity
• Modified Holographic Dark Energy
• Generalized uncertainty principle and Hořava-Lifshitz gravity
• Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields
• Holographic Dark Energy Scenario and Variable Modified Chaplygin Gas
• The black hole horizon as a dynamical system
• $f(R)$ theory and geometric origin of the dark sector in Horava-Lifshitz gravity
• Holographic Dark Energy Model and Scalar-Tensor Theories
• Interacting Ricci Logarithmic Entropy Corrected Holographic Dark Energy in Brans-Dicke Cosmology