Observational Constraints on Hybrid Scale Factor in f(Q,T) Gravity with Anisotropic Space-Time
arXiv:2306.14502 · doi:10.1002/andp.202300161
Abstract
In this paper, we present an accelerating cosmological model by constraining the free parameters using the cosmological datasets in an extended symmetric teleparallel gravity for the flat and anisotropic space-time. We employ a time variable deceleration parameter that behaves early deceleration and late time acceleration in the form of Hybrid Scale Factor (HSF). We obtain the present values of deceleration parameter and analyse the late time behavior of the Universe based on the best-fit values of free parameters. We derive the dynamical parameters of the model and obtain the equation of state parameter at present in the quintessence region; however at late time it approaches to CDM. The energy conditions are also analysed to validate the modified gravity and we find that strong energy condition is violating. We establish the importance of hybrid scale factor in the late time cosmic phenomena issue.
Annalen Der Physik published version
References in corpus (31)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- Extended Gravity Cosmography
- Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
- Correcting Type Ia Supernova Distances for Selection Biases and Contamination in Photometrically Identified Samples
- Signatures of -gravity in cosmology
- Reconstruction of the deceleration parameter and the equation of state of dark energy
- Bouncing Cosmology in f(Q) Symmetric Teleparallel Gravity
- Cosmic Microwave Background Quadrupole and Ellipsoidal Universe
- Cosmographic bounds on the cosmological deceleration-acceleration transition redshift in gravity
- Ellipsoidal Universe Can Solve The CMB Quadrupole Problem
- Spherically symmetric configuration in gravity
- Anisotropic nature of space-time in gravity
- Matter Bounce Scenario and the Dynamical aspects in f(Q,T) Gravity
- Dynamical system analysis for accelerating models in non-metricity gravity
- Cosmological Inflation in f(Q, T) Gravity
- Physics in the Real Universe: Time and Spacetime
- Bianchi Type VII_h Models and the WMAP 3-year Data
- Fast and Efficient Template Fitting of Deterministic Anisotropic Cosmological Models Applied to WMAP Data
- Late-time acceleration in gravity: Analysis and constraints in an anisotropic background
- Model parameters in the context of late time cosmic acceleration in gravity
- Accelerating Universe scenario in anisotropic cosmology
- Thermodynamical aspects of Bianchi type-I Universe in quadratic form of gravity and observational constraints
- Quintessence Universe and cosmic acceleration in gravity
- Constraining the anisotropy of the Universe via Pantheon supernovae sample
- First measurement of the Hubble parameter from bright binary black hole GW190521
- Viscous Dark Energy In Bianchi Type V Space-Time
- Anisotropic Universe in gravity, a novel study
- Theoretic Limits on the Equation of State Parameter of Quintessence
- Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data