2018
DOI: 10.1140/epjc/s10052-018-6233-y
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The observational constraints on the flat $$\phi $$CDM models

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 upcomi… Show more

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Cited by 13 publications
(15 citation statements)
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“…Observational constraints on scalar field cosmological models have been recently investigated in [2]. Using the Bayesian methods different models of the scalar field cosmology were analysed.…”
Section: Introductionmentioning
confidence: 99%
“…Observational constraints on scalar field cosmological models have been recently investigated in [2]. Using the Bayesian methods different models of the scalar field cosmology were analysed.…”
Section: Introductionmentioning
confidence: 99%
“…V φ , ten different quintessence models are suggested by [36]. Here we start from Equation (12) in [37] where…”
Section: ϕCdm Cosmologymentioning
confidence: 99%
“…Primordial magnetic fields are the subject of research which includes main characteristics of inflational magnetic field evolution (Brandenburg et al 2017, their statistical properties and applications to cosmology (Brandenburg et al 2018). The dark energy models are studied and their testings are carried out (Avsajanishvili et al 2017, Avsajanishvili et al 2018).…”
Section: Theoretical Astrophysicsmentioning
confidence: 99%