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• W2729494996 abstract "We do a comprehensive study of the Bayesian evidences for a large number of dark energy models using a combination of latest cosmological data from SNIa, CMB, BAO, strong lensing time delay, growth measurements, measurements of Hubble parameter at different redshifts and measurements of angular diameter distance by Megamaser Cosmology Project. We consider a variety of scalar field models with different potentials as well as different parametrizations for the dark energy equation of state. Among 21 models that we consider in our study, we do not find strong evidences in favor of any evolving dark energy model compared to $mathrm{ensuremath{Lambda}}mathrm{CDM}$. For the evolving dark energy models, we show that purely nonphantom models have much better evidences compared to those models that allow both phantom and nonphantom behaviors. Canonical scalar field with exponential and tachyon field with square potential have highest evidences among all the models considered in this work. We also show that a combination of low redshift measurements decisively favors an accelerating $mathrm{ensuremath{Lambda}}mathrm{CDM}$ model compared to a nonaccelerating power law model." @default.
• W2729494996 created "2017-07-14" @default.
• W2729494996 creator A5024564709 @default.
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• W2729494996 creator A5057167259 @default.
• W2729494996 creator A5069411887 @default.
• W2729494996 creator A5088528226 @default.
• W2729494996 date "2018-02-21" @default.
• W2729494996 modified "2023-10-02" @default.
• W2729494996 title "Bayesian evidences for dark energy models in light of current observational data" @default.
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• W2729494996 doi "https://doi.org/10.1103/physrevd.97.043524" @default.
• W2729494996 hasPublicationYear "2018" @default.
• W2729494996 type Work @default.
• W2729494996 sameAs 2729494996 @default.

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