The evidence of cosmic acceleration and observational constraints
Yingjie Yang, Yungui Gong

TL;DR
This paper provides strong observational evidence for cosmic acceleration using supernovae and cosmic chronometers data, constrains the transition redshift, and confirms the effectiveness of compressed data in cosmological analysis.
Contribution
It offers new evidence for cosmic acceleration, refines the transition redshift, and demonstrates that compressed expansion rate data can replace full supernova datasets.
Findings
> 3σ evidence of cosmic acceleration from multiple data sources
Transition redshift z_t ≈ 0.60-0.61 where acceleration transitions to deceleration
Hubble constant H_0 ≈ 67.5 km/s/Mpc consistent with Planck 2018
Abstract
Directly comparing the 6 expansion rate measured by type Ia supernovae data and the lower bound on the expansion rate set by the strong energy conditions or the null hypothesis that there never exists cosmic acceleration, we see direct evidence of cosmic acceleration and the model is strongly excluded by the type Ia supernovae data. We also use Gaussian process method to reconstruct the expansion rate and the deceleration parameter from the 31 cosmic chronometers data and the 6 data points on the expansion rate measured from type Ia supernoave data, the direct evidence of cosmic acceleration is more than and we find that the transition redshift at which the expansion of the Universe underwent the transition from acceleration to deceleration. The Hubble constant inferred from the cosmic chronometers data with the Gaussian process…
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