Observational Tests of Gauss-Bonnet Like Dark Energy Model

Abstract

The consistency of some dynamical dark energy models based on Gauss-Bonnet invariant, $\mathcal{G}$, is studied compared with cosmological observational tests. The investigated models are modified form of Gauss Bonnet dark energy, MGB-DE and two other versions which are interacting MGB and $n_0$MGB. The energy density of proposed models are combinations of powers of the Hubble rate, H, and its time derivative. To inquire the performance of MGB dark energy models, we have used data analyzing methods and numerical solutions, in both background and perturbed levels, based on recent observational data from SNIa, Baryon Acoustic Oscillations (BAO), Hubble parameter, CMB data, and structure formation data surveys. Employing joint data sets and comparing the results to those of LCDM, show that all versions of MGB-DE predicts the expansion history and evolution of structures appropriately as well as $\Lambda$CDM. If we use pure late universe data set, we see that all models of MGB-DE are successful in recent epoch, and there is not any significant evidence against or in favor of $\Lambda$CDM, whereas for early universe, statistical results indicate a significantly better agreement for $\Lambda$CDM as compared to all versions of MGB-DE models.

arXiv comment19 pages, 6 figures

References in corpus (69)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Dynamics of dark energy
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• f(R) Theories Of Gravity
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• f(R) theories
• Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
• Baryonic Features in the Matter Transfer Function
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
• f(T) teleparallel gravity and cosmology
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Cosmological Constraints from the SDSS Luminous Red Galaxies
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters
• The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
• Small Scale Cosmological Perturbations: An Analytic Approach
• Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample
• Brane-World Gravity
• The Third Data Release of the Sloan Digital Sky Survey
• Gauss-Bonnet dark energy
• Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
• A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - I : Methods and Application to the Sloan Digital Sky Survey
• A test of the nature of cosmic acceleration using galaxy redshift distortions
• Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
• Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes
• The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
• The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering
• Dark energy cosmology from higher-order, string-inspired gravity and its reconstruction
• Reconstructing the history of structure formation using redshift distortions
• Interpreting large-scale redshift-space distortion measurements
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z=0.8 in the first data release
• Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity
• The 2dF Galaxy Redshift Survey: Spherical Harmonics analysis of fluctuations in the final catalogue
• First evidence of running cosmic vacuum: challenging the concordance model
• Our World as an Expanding Shell
• The growth rate of cosmic structure from peculiar velocities at low and high redshifts
• Four Dimensionality in Non-compact Kaluza-Klein Model
• Decaying Vacuum Energy and Deflationary Cosmology in Open and Closed Universes
• Expansion History with Decaying Vacuum: A Complete Cosmological Scenario
• Hints of dynamical vacuum energy in the expanding Universe
• Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
• Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
• Complete Cosmic History with a dynamical Lambda(H) term
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies
• Growth rate of cosmological perturbations at z ~ 0.1 from a new observational test
• Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
• Generalized $f(R,\varphi ,X)$ gravity and the late-time cosmic acceleration
• Constraining $f(R)$ gravity by the Large Scale Structure
• Constraining f(T) gravity in the Solar System
• Ricci-Gauss-Bonnet holographic dark energy
• Holographic thermalization in Gauss-Bonnet gravity
• The cosmology of an holographic induced gravity model with curvature effects
• Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy
• From inflation to dark energy through a dynamical Lambda: an attempt at alleviating fundamental cosmic puzzles
• Holographic Isotropisation in Gauss-Bonnet Gravity
• The holographic induced gravity model with a Ricci dark energy: smoothing the little rip and big rip through Gauss-Bonnet effects?
• Gauss-Bonnet correction to Holographic thermalization: two-point functions, circular Wilson loops and entanglement entropy
• Dark Energy from Gauss-Bonnet and non-minimal couplings
• Agegraphic reconstruction of modified $F(R)$ and $F(\mathcal{G})$ gravities
• Natural scaling for dark energy
• Holography in Einstein Gauss-Bonnet Gravity
• Running of the Spectral index in Deformed Matter Bounce Scenarios with Hubble-rate-dependent Dark Energy
• Gauss Bonnet dark energy Chaplygin Gas Model

Cited by in corpus (13)

• Barrow holographic dark energy
• Barrow holographic dark energy with Hubble horizon as IR cutoff
• Unified Dark Energy and Dark Matter from Dynamical Space Time
• Data Analysis of three parameter models of deceleration parameter in FRW Universe
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Diagnostic and Comparative Analysis of Dark Energy Models with $q(z)$ Parametrizations
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Interacting Barrow Holographic Dark Energy in Non-flat Universe
• Mimetic Tensor-Vector-Scalar Cosmology: Incorporating Dark Matter, Dark Energy and Stiff Matter
• Friedmann's Universe Controlled by Gauss-Bonnet Modified Gravity