Stability analysis in Modified Non-Local Gravity
arXiv:1103.3553 · doi:10.1007/s10773-011-0710-5
Abstract
In this paper we consider FRW cosmology in modified non-local gravity. The stability analysis shows that there is only one stable critical point for the model and the universe undergoes a quintessence dominated era.
12 pages, 4 figures, will be published in Int. J. Theor. Phys
References in corpus (78)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Cosmological parameters from SDSS and WMAP
- 4D Gravity on a Brane in 5D Minkowski Space
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- The 3D power spectrum of galaxies from the SDSS
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Cosmological Results from High-z Supernovae
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Kinetically Driven Quintessence
- The Second Data Release of the Sloan Digital Sky Survey
- Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Reconstruction of a scalar-tensor theory of gravity in an accelerating universe
- Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters
- 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
- The Third Data Release of the Sloan Digital Sky Survey
- Braneworld models of dark energy
- Unifying inflation with LambdaCDM epoch in modified f(R) gravity consistent with Solar System tests
- Curvature quintessence matched with observational data
- Do consistent models mimic General Relativity plus ?
- Cosmological Dynamics of Phantom Field
- A Parameterized Post-Friedmann Framework for Modified Gravity
- Modified gravity and its reconstruction from the universe expansion history
- Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
- Matter density perturbations and effective gravitational constant in modified gravity models of dark energy
- Interacting holographic dark energy model in non-flat universe
- Modified non-local-F(R) gravity as the key for the inflation and dark energy
- Interacting holographic generalized Chaplygin gas model
- Quintessence and phantom cosmology with non-minimal derivative coupling
- The Fate of Bound Systems in Phantom and Quintessence Cosmologies
- What does inflation really predict?
- The fate of (phantom) dark energy universe with string curvature corrections
- de Sitter space and the equivalence between f(R) and scalar-tensor gravity
- A unified approach to scaling solutions in a general cosmological background
- Cosmological Constraints on f(R) Acceleration Models
- Newton law corrections and instabilities in gravity with the effective cosmological constant epoch
- Phantom and non-phantom dark energy: The cosmological relevance of non-locally corrected gravity
- Crossing of the phantom divide in modified gravity
- Interacting generalized Chaplygin gas model in non-flat universe
- Correspondence between Holographic and Gauss-Bonnet dark energy models
- Nearly Scale-Invariant Spectrum of Adiabatic Fluctuations May be from a Very Slowly Expanding Phase of the Universe
- Interacting Phantom Energy
- Quintom model with O() symmetry
- The phase space view of f(R) gravity
- Exactly Solvable SFT Inspired Phantom Model
- Can we be tricked into thinking that w is less than -1?
- Can f(R) Modified Gravity Theories Mimic a LCDM Cosmology?
- Non-minimally Coupled Quintom Model Inspired by String Theory
- Constraints on coupling constant between dark energy and dark matter
- Cosmology as Geodesic Motion
- On the resolution of cosmic coincidence problem and phantom crossing with triple interacting fluids
- Attractors, Statefinders and Observational Measurement for Chameleonic Brans--Dicke Cosmology
- Interacting new generalized Chaplygin gas
- Generalised cosmological scaling solutions
- Cosmic Dynamics in the Chameleon Cosmology
- Reconstructing a String-Inspired Quintom Model of Dark Energy
- A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane
- Bouncing universe with the non-minimally coupled scaler field and its reconstructing
- Quintessence and phantom dark energy from ghost D-branes
- Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
- A single model of interacting dark energy: generalized phantom energy or generalized Chaplygin gas
- Generalized Brans-Dicke cosmology in the presence of matter and dark energy
- Interacting Cosmic Fluids in Brans-Dicke Cosmology
- A 5D noncompact Kaluza -Klein cosmology in the presence of Null perfect fluid
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- Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
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- Dynamical stability in scalar-tensor cosmology