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- W2969801460 abstract "We analyze various low-redshift cosmological data from Type-Ia supernova, baryon acoustic oscillations, time-delay measurements using strong-lensing, $H(z)$ measurements using cosmic chronometers and growth measurements from large scale structure observations for $mathrm{ensuremath{Lambda}}mathrm{CDM}$ and some different dark energy models. By calculating the Bayesian evidence for different dark energy models, we find out that the $mathrm{ensuremath{Lambda}}mathrm{CDM}$ still gives the best fit to the data with ${H}_{0}={70.3}_{ensuremath{-}1.35}^{+1.36}text{ }text{ }mathrm{Km}/mathrm{s}/mathrm{Mpc}$ (at $1ensuremath{sigma}$). This value is in $ensuremath{lesssim}2ensuremath{sigma}$ tension with various low and high redshift measurements for ${H}_{0}$ including SH0ES, Planck-2018 and the recent results from H0LiCOW-XIII. The derived constraint on ${S}_{8}={ensuremath{sigma}}_{8}sqrt{{mathrm{ensuremath{Omega}}}_{m0}/0.3}$ from our analysis is ${S}_{8}=0.7{6}_{ensuremath{-}0.03}^{+0.03}$, fully consistent with direct measurement of ${S}_{8}$ by $mathrm{KiDS}+mathrm{VIKING}ensuremath{-}450+mathrm{DES}1$ survey. We hence conclude that the $mathrm{ensuremath{Lambda}}mathrm{CDM}$ model with parameter constraints obtained in this work is consistent with different early and late Universe observations within $2ensuremath{sigma}$. We therefore, do not find any compelling reason to go beyond concordance $mathrm{ensuremath{Lambda}}mathrm{CDM}$ model." @default.
- W2969801460 created "2019-08-29" @default.
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- W2969801460 date "2019-11-01" @default.
- W2969801460 modified "2023-10-03" @default.
- W2969801460 title "Cosmology with low-redshift observations: No signal for new physics" @default.
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- W2969801460 doi "https://doi.org/10.1103/physrevd.100.103501" @default.
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