Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
arXiv:1403.6178 · doi:10.1007/s10714-014-1789-9
Abstract
In this study, FRW cosmology in modified gravity containing arbitrary function is taken into consideration when our action are coupled with Weyl tensor. It is indicated that the bouncing solution emerges in the model while the equation of state (EoS) parameter crosses the phantom divider. In this research, cosmological usage of the most promising candidates of dark energy in the framework of theory coupled by Weyl tensor is explored. A gravity model in the spatially flat FRW universe according to the ordinary version of the holographic dark energy model, which describes accelerated expansion of the universe is reconstructed. The equation of state parameter of the corresponding Weyl gravity models are obtained as well. We conclude that the holographic and Weyl gravity models can behave like phantom or quintessence models, whereas the equation of state parameter of the models can transit from quintessence state to phantom regime as shown recent observations.
arXiv comment18 Pages, 1 figure. arXiv admin note: text overlap with arXiv:1004.1805 by other authors
References in corpus (116)
- 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
- The Cosmological Constant and 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
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- 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
- Cosmology and the Fate of Dilatation Symmetry
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Phantom Energy and Cosmic Doomsday
- 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
- A Model of Holographic Dark Energy
- 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
- New Constraints on , , and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
- Kinetically Driven Quintessence
- Dark Energy Constraints from the Cosmic Age and Supernova
- Can the dark energy equation-of-state parameter w be less than -1?
- 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
- Extra force in modified theories of gravity
- Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
- The First Data Release of the Sloan Digital Sky Survey
- 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
- BVRI Light Curves for 22 Type Ia Supernovae
- 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
- The phantom menaced: constraints on low-energy effective ghosts
- Scaling solutions in general non-minimal coupling theories
- 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 scaling solutions of non-minimally coupled scalar fields
- Modified f(R) gravity unifying R^m inflation with \LambdaCDM epoch
- The State of the Dark Energy Equation of State
- One-loop f(R) gravity in de Sitter universe
- Modified gravity with terms and cosmic acceleration
- Extended Quintessence
- Where new gravitational physics comes from: M-theory?
- Modified gravity and its reconstruction from the universe expansion history
- The case for dynamical dark energy revisited
- Gravity assisted dark energy dominance and cosmic acceleration
- The Power of General Relativity
- Quintessence, the Gravitational Constant, and Gravity
- The Cosmology of f(R) Gravity in the Metric Variational Approach
- Matter density perturbations and effective gravitational constant in modified gravity models of dark energy
- Scalar-Tensor Gravity and Quintessence
- Energy conditions in f(R)-gravity
- Phantom scalar dark energy as modified gravity: understanding the origin of the Big Rip singularity
- Modified non-local-F(R) gravity as the key for the inflation and dark energy
- Phantom crossing, equation-of-state singularities, and local gravity constraints in f(R) models
- The dS/CFT Correspondence and the Big Smash
- Holographic dark energy models: A comparison from the latest observational data
- Bounce cosmology from gravity and bigravity
- Constraints on linear-negative potentials in quintessence and phantom models from recent supernova data
- The Fate of Bound Systems in Phantom and Quintessence Cosmologies
- A f(R) gravity without cosmological constant
- Cosmological observations in scalar-tensor quintessence
- What does inflation really predict?
- Quintessence, super-quintessence and observable quantities in Brans-Dicke and non-minimally coupled theories
- The fate of (phantom) dark energy universe with string curvature corrections
- B-Inflation
- Solar System experiments do not yet veto modified gravity models
- Fourth order gravity: equations, history, and applications to cosmology
- A unified approach to scaling solutions in a general cosmological background
- The evolution of density perturbations in f(R) gravity
- Crossing the Phantom Divide Barrier with Scalar Tensor Theories
- Dark energy from modified F(R)-scalar-Gauss-Bonnet gravity
- Static spherically symmetric perfect fluid solutions in theories of gravity
- Cosmological Constraints on f(R) Acceleration Models
- Are galactic rotation curves really flat?
- Newton law corrections and instabilities in gravity with the effective cosmological constant epoch
- Viability of f(R) Theories with Additional Powers of Curvature
- The Phantom Divide in String Gas Cosmology
- Interacting Phantom Energy
- The phase space view of f(R) gravity
- Modified gravity as an alternative for Lambda-CDM cosmology
- Conformal transformations in classical gravitational theories and in cosmology
- 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
- Black hole entropy in modified gravity models
- The Limits of Extended Quintessence
- Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models
- Stellar configurations in f(R) theories of gravity
- Cosmology as Geodesic Motion
- Modified gravity with
- Generalised cosmological scaling solutions
- Phantom-Like Behavior in -Gravity
- The accelerating universe and a limiting curvature proposal
- Bouncing universe with the non-minimally coupled scaler field and its reconstructing
- Early and Late Transient Cosmic Acceleration due to Curvature Inspired Dark Energy
- Cosmic Dynamics in Gravity
- Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
- An Inverse Gravitation for Cosmic Speed up, and Dark Energy Equivalent
- Stability analysis in Modified Non-Local Gravity
- Cosmological observations in non-local cosmology