Revisiting cosmography via Gaussian process

Abstract In this paper, we revisit the kinematical state of our Universe via the cosmographic approach by using Gaussian process, where the minimum assumption is the cosmological principle, i. e. the Friedmann–Lemaître–Robertson–Walker metric. A obviously distinguished feature is that these cosmography parameters are free of any gravity theories and cosmological models. And Gaussian process is independent of any specific parameterized forms of function. Thus by transformations these generic cosmography parameters can be used to constrain a cosmological model and dark energy model directly at the kinematics level of our Universe. As a result, a series of cosmography parameters up to the fifth oder, i. e. the Hubble parameter H (z), the deceleration parameter q (z), the jerk parameter j (z), the snap parameter s (z) and the lerk parameter l (z), evolve with respect to the redshift z are reconstructed from the cosmic observations which include the recently released Pantheon+ SN Ia samples and the observational Hubble data H (z), also dubbed as cosmic chronometers. The result shows the transition redshift from a decelerated expansion to an accelerated expansion zₜ=0. 652^+0. 054-₀. ₀₄₃ z t = 0. 652 - 0. 043 + 0. 054 which is consistent with the previous results.