A parametric reconstruction of the cosmological jerk from diverse observational data sets
arXiv:1601.05172 · doi:10.1103/PhysRevD.93.043002
Abstract
A parametric reconstruction of the jerk parameter, the third order derivative of the scale factor expressed in a dimensionless way, has been discussed. Observational constraints on the model parameters have been obtained by Maximum Likelihood Analysis of the models using Supernova Distance Modulus data (SNe), Observational Hubble Data (OHD), Baryon Acoustic Oscillation (BAO) data and CMB shift parameter data (CMBShift). The present value of the jerk parameter has been kept open to start with, but the plots of various cosmological parameter like deceleration parameter , jerk parameter , dark energy equation of state parameter indicate that the reconstructed models are very close to a CDM model with a slight inclination towards a non-phantom behaviour of the evolution.
12 pages, 44 figures; Accepted for publication in Phys. Rev. D
References in corpus (12)
- Dynamics of dark energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- Reconstructing Dark Energy
- A kinematical approach to dark energy studies
- Thawing quintessence with a nearly flat potential
- Reconstruction of the deceleration parameter and the equation of state of dark energy
- Nonparametric Reconstruction of the Dark Energy Equation of State
- Cosmic Jerk, Snap and Beyond
- Phantom Dark Energy Models with a Nearly Flat Potential
- Quintessence reconstructed: new constraints and tracker viability
- Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
Cited by in corpus (37)
- Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
- Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
- Dark energy models from a parametrization of : A comprehensive analysis and observational constraints
- A Comparison of Thawing and Freezing Dark Energy Parametrizations
- In search of the dark matter dark energy interaction: a kinematic approach
- Acceleration of the universe: a reconstruction of the effective equation of state
- Non-parametric reconstruction of the cosmological \textit{jerk} parameter
- Phantom cosmological model with observational constraints in gravity
- Geodesics and the magnitude-redshift relation on cosmologically symmetric Finsler spacetimes
- Real-time cosmography with redshift derivatives
- Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
- Constraining the dark energy models with H(z) data: an approach independent of
- Constraining the Asymptotically Safe Cosmology: cosmic acceleration without dark energy
- Model selection applied to reconstructions of the Dark Energy
- Cosmological implications of the constant jerk parameter in gravity theory
- Constraining the dark energy statefinder hierarchy in a kinematic approach
- Reconstruction of gravity models for an accelerated universe using Raychaudhuri equation
- Isolating the Lyman Alpha Forest BAO Anomaly
- Reconstruction of interaction rate in Holographic dark energy
- On Reconstruction of Extended Teleparallel Gravity from the Cosmological Jerk Parameter
- Mori-Zwanzig formalism for general relativity: a new approach to the averaging problem
- A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
- Recovering CDM Model From a Cosmographic Study
- Cosmological model with linear equation of state parameter in f(R, Lm) gravity
- A generalized CDM model with parameterized Hubble parameter in particle creation, viscous and model framework
- Cosmic jerk parameter in symmetric teleparallel cosmology
- Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
- On the uniqueness of CDM-like evolution for homogeneous and isotropic cosmology in General Relativity
- Cosmic Acceleration in an Extended Brans-Dicke-Higgs Theory
- An exact solution of the observable universe in Bianchi V space-time
- Density perturbation in the models reconstructed from jerk parameter
- Reconstructing cosmic evolution with a density parametrization
- Kinematical models of latetime cosmology and the statefinder diagnostic
- Reconstruction of Tsallis Holographic Dark Energy via Modified Non-Metric Gravity: An Approach
- Perturbations In Some Dark Energy Models
- On Generalized Theories of Varying Fine Structure Constant
- The gravity and affine EoS: Compatibility and observational constraints