Cosmography with DESI DR2 and SN data

TL;DR

This study uses cosmography with DESI DR2 and supernova data to analyze the universe's expansion, finding potential evidence for dynamic dark energy beyond the standard Lambda-CDM model.

Contribution

It provides a model-independent cosmographic analysis combining DESI DR2 and SN data, revealing significant deviations from Lambda-CDM predictions.

Findings

DESI DR2 data alone is consistent with Lambda-CDM within 2σ.

Combined SN datasets show deviations from Lambda-CDM at over 3σ.

Results support the possibility of a dynamic dark energy component.

Abstract

In this paper, we present a kinematic analysis of the Universe's expansion history using cosmography, with a particular emphasis on the jerk parameter $j_0$, which is equal to one in the standard $\Lambda$CDM scenario. We use distance measurements from DESI DR2, both independently and in combination with current Type Ia supernova (SN) samples, to constrain the cosmographic parameters up to the fourth order without relying on a specific cosmological model. Our results show that for the DESI DR2 data alone, the $\Lambda$CDM prediction ($j_0 = 1$) falls within the 2$\sigma$ confidence region. However, when DESI DR2 is combined with the Union3, Pantheon+, and DESY5 SN datasets, the result obtained is discrepant with the $\Lambda$CDM model at about 3.4$\sigma$, 4.1$\sigma$, and 5.4$\sigma$, respectively. These results are consistent with the conclusions based on dark energy parameterizations reported by the DESI Collaboration, which suggest the presence of a dynamic dark energy component in the universe.