Eur. Phys. J. C (2018) 78: 773
https://doi.org/10.1140/epjc/s10052-018-6233-y

Regular Article - Theoretical Physics

The observational constraints on the flat CDM models

¹ Abastumani Astrophysical Observatory, Ilia State University, 3-5 Cholokashvili Ave., 0194, Tbilisi, Georgia
² Department of Physics, University of California, San Diego, La Jolla, CA, 92093, USA
³ Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS, 66506, USA
⁴ McWilliams Center for Cosmology and Department of Physics, Carnegie Mellon University, 5000 Forbes Ave, Pittsburgh, PA, 15213, USA
⁵ Department of Physics, Laurentian University, Ramsey Lake Road, Sudbury, ON, P3E 2C, Canada

^* e-mail: olga.avsajanishvili@iliauni.edu.ge

Received: 28 March 2018
Accepted: 10 September 2018
Published online: 26 September 2018

Abstract

Most dark energy models have the CDM as their limit, and if future observations constrain our universe to be close to CDM Bayesian arguments about the evidence and the fine-tuning will have to be employed to discriminate between the models. Assuming a baseline CDM model we investigate a number of quintessence and phantom dark energy models, and we study how they would perform when compared to observational data, such as the expansion rate, the angular distance, and the growth rate measurements, from the upcoming Dark Energy Spectroscopic Instrument (DESI) survey. We sample posterior likelihood surfaces of these dark energy models with Monte Carlo Markov Chains while using central values consistent with the Planck CDM universe and covariance matrices estimated with Fisher information matrix techniques. We find that for this setup the Bayes factor provides a substantial evidence in favor of the CDM model over most of the alternatives. We also investigated how well the CPL parametrization approximates various scalar field dark energy models, and identified the location for each dark energy model in the CPL parameter space.