Observational Constraint in gravity from the cosmic chronometers and some standard distance measurement parameters
arXiv:2009.14630 · doi:10.1016/j.nuclphysb.2021.115428
Abstract
In this work we perform an observational data analysis on the gravity with the aim of constraining the parameter space of the model. Five different models are considered and the 30 point cosmic chronometer data is used in our analysis. The statistic is formulated as a difference between the theoretical and the observed values of for different values of redshift . Efforts have been made to minimize the statistic in order to get the best fit values for the free parameters models. We have also used some standard distance measurement parameters like BAO and CMB peaks along with the data for achieving better constraints on the parameter space. We have used the publicly available \textit{CosmoMC} code for obtaining the bounds for the free parameters of the models in different confidence intervals like , , . 1D distributions and 2D joint confidence contours for various confidence levels mentioned above are generated for the free parameters using the \textit{CosmoMC} code. Finally our models have been compared with the standard model by some statistical techniques using the observational data and the support for the models from the data is probed.
arXiv comment20 pages, 10 figures
References in corpus (41)
- 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
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Efficient Computation of CMB anisotropies in closed FRW models
- f(R) Theories Of Gravity
- f(R) theories
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- f(R,T) gravity
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Constraints on the redshift dependence of the dark energy potential
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Constraining Cosmological Parameters Based on Relative Galaxy Ages
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Conditions for the cosmological viability of f(R) dark energy models
- Scaling solutions in general non-minimal coupling theories
- f(R,L_m) gravity
- Are f(R) dark energy models cosmologically viable ?
- The Large Scale Structure of f(R) Gravity
- Cosmological scaling solutions of non-minimally coupled scalar fields
- Dynamics of scalar perturbations in f(R,T) gravity
- f(R,T) Cosmological Models in Phase Space
- Quintessence, super-quintessence and observable quantities in Brans-Dicke and non-minimally coupled theories
- Dark Matter From f(R,T) Gravity
- Gravastars in gravity
- Is the Jeffreys' scale a reliable tool for Bayesian model comparison in cosmology?
- Accelerated expansion from a non-minimal gravitational coupling to matter
- Matter density perturbations in modified gravity models with arbitrary coupling between matter and geometry
- Galactic rotation curves in modified gravity with non-minimal coupling between matter and geometry
- Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
- Reheating via a generalized non-minimal coupling of curvature to matter
- Modified Chaplygin Gas and Constraints on its B parameter from CDM and UDME Cosmological models
- Constraints on Exotic Matter for An Emergent Universe
- Propagation of Polar Gravitational Waves in f(R,T) Scenario
- Can structure formation distinguish ΛCDM from non-minimal f(R) Gravity?
- Emergent Universe from A Composition of Matter, Exotic Matter and Dark Energy
- Dynamical analysis of generalised theories
- Thermodynamics in theories: Apparent horizon in the FLRW spacetime
- Cosmological Dynamics of Modified Gravity With a Non-minimal Curvature-matter Coupling
- A Time Dependent Spacetime in Gravity: Gravitational Collapse
Cited by in corpus (13)
- Thermodynamics and Perturbative Analysis of Some Newly Developed Theories Under the Scenario of Conserved Energy-momentum Tensor
- Constraints on Cubic and Gravity from the Cosmic Chronometers, BAO & CMB datasets : Use of Machine Learning Algorithms
- Reconstruction of Lagrangian for various cosmological scenarios
- Energy-momentum squared symmetric Teleparallel gravity: gravity
- Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
- Observational Restrictions and Slow-Roll D-brane Inflation in the Special Gravity
- Analysing Ultra High Energy Cosmic Rays' Anisotropy in Gravity Theory
- Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
- Black holes in gravity coupled with Euler-Heisenberg electrodynamics
- Exact Analytical Taub-NUT like Solution in f(T) Gravity
- Phase space analysis of Bianchi III Universe with gravity theory
- New Lorentzian Taub-NUT and Euclidean Eguchi-Hanson Solutions in gravity
- Exploration of Parameters in f(R,T) Gravity and Comparison with Type Ia Supernovae Data