Constraining Bianchi type V universe with recent H(z) and BAO observations in Brans-Dicke theory of gravitation
arXiv:2003.08734 · doi:10.1140/epjp/s13360-020-00308-9
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 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 . Some physical properties of the universe are also discussed.
17 pages, 8 figures
References in corpus (18)
- Dynamics of dark energy
- 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
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- Baryon Acoustic Oscillations in the Ly-α forest of BOSS quasars
- FRW Cosmology in F(R,T) gravity
- The simplest non-minimal matter-geometry coupling in the cosmology
- Constraints on a Bianchi type I spacetime extension of the standard CDM model
- Dark energy models with variable equation of state parameter
- Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter
- Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology
- Brans-Dicke Theory as a Unified Model for Dark Matter - Dark Energy
- Decaying Gravity
- Viscous Dark Energy In Bianchi Type V Space-Time
- Two Fluid Scenario in Bianchi Type-I Universe
- Invariant Bianchi type I models in Gravity
- Anisotropic massive Brans-Dicke gravity extension of the standard CDM model
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