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• W4311769032 endingPage "4950" @default.
• W4311769032 startingPage "4938" @default.
• W4311769032 abstract "Taking advantage of Gaussian process (GP), we obtain an improved estimate of the Hubble constant, $H_0=70.41pm1.58$ km s$^{-1}$ Mpc$^{-1}$, using Hubble parameter [$H(z)$] from cosmic chronometers (CCH) and expansion rate function [$E(z)$], extracted from type Ia supernovae, data. We also use CCH data, including the ones with full covariance matrix, and $E(z)$ data to obtain a determination of $H_0=72.34_{-1.92}^{+1.90}$ km s$^{-1}$ Mpc$^{-1}$, which implies that the involvement of full covariance matrix results in higher values and uncertainties of $H_0$. These results are higher than those obtained by directly reconstructing CCH data with GP. In order to estimate the potential of future CCH data, we simulate two sets of $H(z)$ data and use them to constrain $H_0$ by either using GP reconstruction or fitting them with $E(z)$ data. We find that simulated $H(z)$ data alleviate $H_0$ tension by pushing $H_0$ values higher towards $sim70$ km s$^{-1}$ Mpc$^{-1}$. We also find that joint $H(z)$ + $E(z)$ data favor higher values of $H_0$, which is also confirmed by constraining $H_0$ in the flat concordance model and 2-order Taylor expansion of $H(z)$. In summary, we conclude that more and better-quality CCH data as well as $E(z)$ data can provide a new and useful perspective on resolving $H_0$ tension." @default.
• W4311769032 created "2022-12-28" @default.
• W4311769032 creator A5006042484 @default.
• W4311769032 creator A5032668167 @default.
• W4311769032 creator A5060378664 @default.
• W4311769032 creator A5077066156 @default.
• W4311769032 date "2022-12-09" @default.
• W4311769032 modified "2023-10-14" @default.
• W4311769032 title "Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension" @default.
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• W4311769032 doi "https://doi.org/10.1093/mnras/stac3617" @default.
• W4311769032 hasPublicationYear "2022" @default.
• W4311769032 type Work @default.
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