Model independent cosmographic constraints from DESI 2024

In this study, we explore model independent constraints on the universe kinematics up to the snap and jerk hierarchical terms. To do so, we consider the latest Baryon Acoustic Oscillation (BAO) release provided by the DESI collaboration, tackling the rd parameter to span within the range $[144,152]$ Mpc, with fixed step, δ rd=2 Mpc, aligning with Planck and DESI results. Thus, employing Monte Carlo Markov chain analyses, we place stringent constraints on the cosmographic series, incorporating three combinations of data catalogs: the first BAO with observational Hubble data, the second BAO with type Ia supernovae, and the last including all three data sets. Our results conclusively constrain the cosmographic series, say the deceleration q₀, the jerk j₀, and the snap s₀ parameters, at the $2$--σ level, showcasing a significant departure on j₀ even at $1$--σ confidence level, albeit being compatible with the ΛCDM paradigm on q₀ and s₀, at $2$--σ level. Analogously, the h₀ tension appears alleviated in the second hierarchy, say including snap. Finally, a direct comparison with the ΛCDM, wCDM models and the Chevallier-Polarski-Linder parametrization is reported, definitively favoring the wCDM scenario.