Cosmography approach to dark energy cosmologies: new constrains using the Hubble diagrams of supernovae, quasars and gamma-ray bursts
arXiv:2008.03092 · doi:10.3847/1538-4357/aba517
Abstract
In the context of cosmography approach and using the data of Hubble diagram for supernovae, quasars and gamma-ray bursts, we study some DE parametrizations and also the concordance CDM universe. Using the different combinations of data sample including ({\it i}) supernovae (Pantheon), ({\it ii}) Pantheon + quasars and ({\it iii}) Pantheon + quasars + gamma-ray bursts and applying the minimization of function of distance modulus of data samples in the context of Markov Chain Monte Carlo method, we first obtain the constrained values of the cosmographic parameters in model independent cosmography scenario. We then investigate our analysis, for different concordance CDM cosmology, CDM, CPL and Pade parametrizations. Comparing the numerical values of the cosmographic parameters obtained for DE scenarios with those of the model independent method, we show that the concordance CDM model has a serious tension when we involve the quasars and gamma-ray bursts data in our analysis. While the high redshift quasars and gamma-ray bursts can falsify the concordance model, our results of cosmography approach indicate that the other DE parametrizations are still consistent with these observations.
Accepted in ApJ
References in corpus (21)
- Dynamics of dark energy
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- The X-ray-to-Optical Properties of Optically-Selected Active Galaxies Over Wide Luminosity and Redshift Ranges
- The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary
- SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes
- The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky Survey
- A time - luminosity correlation for Gamma Ray Bursts in the X - rays
- Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated - correlation
- Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
- A Full Year's Chandra Exposure on SDSS Quasars from the Chandra Multiwavelength Project
- Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
- Connecting early and late epochs by f(z)CDM cosmography
- Accelerating cosmologies tested by distance measures
- The UV Properties of SDSS Selected Quasars
- A Bayesian comparison between CDM and phenomenologically emergent dark energy models
- Agegraphic dark energy: growth index and cosmological implications
- Observational constraints on the oscillating dark energy cosmologies
- Structure formation in dark energy cosmologies described by PADE parameterization