Constraining Bianchi type V universe with recent H(z) and BAO observations in Brans-Dicke theory of gravitation

Abstract

In this paper, we investigate a transitioning model of Bianchi type V universe in Brans-Dicke theory of gravitation. The derived model not only validates Mach's principle but also describes the present acceleration of the universe. In this paper, our aim is to constrain an exact Bianchi type V universe in Brans - Dicke gravity. For this sake, firstly we obtain an exact solution of field equations in modified gravity and secondly constrain the model parameters by bounding the model with recent $H(z)$ and Baryon acoustic oscillations (BAO) observational data. The current phase of accelerated expansion of the universe is also described by the contribution coming from cosmological constant screened scalar field with deceleration parameter showing a transition redshift of about $z_t=0.79$. Some physical properties of the universe are also discussed.

arXiv comment17 pages, 8 figures

References in corpus (57)

• 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
• Dynamics of dark energy
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Statefinder -- a new geometrical diagnostic of dark energy
• Constraints on the redshift dependence of the dark energy potential
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
• Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2
• Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers
• The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1
• Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic
• Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
• Cosmological implications of baryon acoustic oscillation (BAO) measurements
• Clustering of Luminous Red Galaxies IV: Baryon Acoustic Peak in the Line-of-Sight Direction and a Direct Measurement of H(z)
• Baryon Acoustic Oscillations in the Ly-α forest of BOSS quasars
• Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope
• The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
• Reconstruction of f(R, T) gravity describing matter dominated and accelerated phases
• The WiggleZ Dark Energy Survey: Improved Distance Measurements to z = 1 with Reconstruction of the Baryonic Acoustic Feature
• Nonminimal coupling and quintessence
• Modeling the Anisotropic Two-Point Galaxy Correlation Function on Small Scales and Improved Measurements of H(z), D_A(z), and f(z)sigma_8(z) from the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
• Cosmic acceleration without quintessence
• FRW Cosmology in F(R,T) gravity
• The simplest non-minimal matter-geometry coupling in the $f(R,T)$ cosmology
• LRS Bianchi Type I Models with Anisotropic Dark Energy and Constant Deceleration Parameter
• Late time acceleration in Brans Dicke Cosmology
• Median statistics and the Hubble constant
• Determining the Hubble constant from Hubble parameter measurements
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Dark energy models with variable equation of state parameter
• Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Some Anisotropic Dark Energy Models in Bianchi Type-V Space-time
• Some Bianchi Type-V Models of Accelerating Universe with Dark Energy
• Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology
• Energy conditions in $F(T,\Theta )$ gravity and compatibility with a stable de Sitter solution
• Decaying Gravity
• Brans-Dicke Theory as a Unified Model for Dark Matter - Dark Energy
• Interacting new agegraphic dark energy in non-flat Brans-Dicke cosmology
• Bianchi-V string cosmology with power law expansion in $f(R,T)$ Gravity
• Probing Dark Energy in The scope of Bianchi type I Spacetime
• Multiband Diagnostics of Unidentified 1FGL Sources with Suzaku and Swift X-ray Observations
• Viscous Dark Energy In Bianchi Type V Space-Time
• A transitioning universe with anisotropic dark energy
• Two Fluid Scenario in Bianchi Type-I Universe
• Invariant Bianchi type I models in $f\left(R,T\right)$ Gravity
• Anisotropic massive Brans-Dicke gravity extension of the standard $\Lambda$CDM model
• Transitioning scenario of Bianchi-I universe within $f\left(R,T\right)$ formalism
• Evolution of the Cosmological Horizons in a Universe with Countably Infinitely Many State Equations
• Some Cosmological Consequences of Non Trivial PPN Parameters $\beta$ and $\gamma$
• A Comparison of the LVDP and ΛCDM Cosmological Models

Cited by in corpus (6)

• An Axially Symmetric Transitioning models with Observational Constraints
• Transitioning Universe with hybrid scalar field in Bianchi I space-time
• Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
• The simplest parametrization of equation of state parameter in the scalar field Universe
• An exact solution of the observable universe in Bianchi V space-time
• Accelerating Universe with binary mixture of bulk viscous fluid and dark energy