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Rui-Yun Guo, Jing-Fei Zhang, and Xin Zhang, “Can the H 0 H_{0} tension be resolved in extensions to Λ \Lambda CDM cosmology?” JCAP 02
Original
2019
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Weiqiang Yang, Supriya Pan, Eleonora Di Valentino, Emmanuel N. Saridakis, and Subenoy Chakraborty, “Observational constraints on one-parameter dynamical dark-energy parametrizations and the H 0 H_{0} tension,” Phys. Rev. D 99
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2019
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N. Aghanim et al. (Planck), “Planck 2018 results. VI. Cosmological parameters,” Astron. Astrophys. 641
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2020
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Suhail Dhawan, Justin Alsing, and Sunny Vagnozzi, “Non-parametric spatial curvature inference using late-Universe cosmological probes,” Mon. Not. Roy. Astron. Soc. 506
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2021
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2024

Measuring cosmic curvature with non-CMB observations

Wu, Peng-Ju, Zhang, Xin

Understand

The cosmic curvature $\Omega_{K}$ is an important parameter related to the inflationary cosmology and the ultimate fate of the universe.

In this work, we adopt the non-CMB observations to constrain $\Omega_{K}$ in the $\Lambda$CDM model and its extensions.
The DESI baryon acoustic oscillation, DES type Ia supernova, cosmic chronometer, and strong gravitational lensing time delay data are considered.
We find that the data combination favors an open universe in the $\Lambda$CDM model, specifically $\Omega_{K}=0.108\pm0.056$ at the $1\sigma$ confidence level, which is in $2.6\sigma$ tension with the Planck CMB result supporting our universe being slightly closed.