Inferring the Age of the Universe with Globular Clusters
David Valcin, Jos\'e Luis Bernal, Raul Jimenez, Licia Verde, Benjamin, D. Wandelt

TL;DR
This paper estimates the age of the Universe by analyzing the color-magnitude diagrams of 68 globular clusters, providing a model-independent age consistent with cosmological measurements.
Contribution
It introduces a novel method to robustly estimate globular cluster parameters from color-magnitude diagrams using priors, leading to an independent universe age estimate.
Findings
Oldest globular clusters have an average age of 13.32 Gyr.
Estimated universe age is 13.5 Gyr, consistent with Planck results.
Distances agree with Gaia measurements.
Abstract
We present an estimate of the absolute age of 68 galactic globular clusters obtained by exploiting the distribution of stars in the full color-magnitude diagram. In particular, we jointly estimate the absolute age, distance, reddening, metallicity ([Fe/H]) and [/Fe] of each cluster, imposing priors motivated by independent observations; we also estimate possible systematics from stellar modeling. Our derived distances for the globular cluster sample are in agreement with those obtained from GAIA using main-sequence dwarf stars (where available), and the inferred ages are in good agreement with those previously published. The novelty of our approach is that, with the adopted priors, we are able to estimate robustly these parameters from the globular cluster color-magnitude diagram. We find that the average age of the oldest globular clusters is $t_{\rm GC}=13.32 \pm 0.1 {\rm…
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