Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
Jun-Jie Wei, Fulvio Melia

TL;DR
This study uses ages of old astrophysical objects and supernova data to investigate the Hubble tension and spatial curvature, finding a possible slight deviation from flatness and constraints on H0 that relate to existing tensions.
Contribution
It provides new constraints on H0 and spatial curvature using age data, highlighting the dependence on priors and comparing different cosmological models.
Findings
Upper limit on H0 is 70.6 km/s/Mpc at 95% CL.
The data favor the R_h=ct universe over Einstein-de Sitter.
Spatial curvature is marginally consistent with flatness at 1.6 sigma.
Abstract
We use the age measurements of 114 old astrophysical objects (OAO) in the redshift range to explore the Hubble tension. The age of the Universe at any is inversely proportional to the Hubble constant, , so requiring the Universe to be older than the OAO it contains at any will lead to an upper limit on . Assuming flat CDM and setting a Gaussian prior on the matter density parameter informed by {\it Planck}, we obtain a 95\% confidence-level upper limit of , representing a tension with the measurement using the local distance ladder. We find, however, that the inferred upper limit on depends quite sensitively on the prior for , and the Hubble tension between early-time and local measurements of may be due in part to the…
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