No evidence of beyond soft corrections to the Born Infeld paradigm in the cosmic history
The Dieterici fluid model can be applied for describing the growth of the dark energy amount and the expenses of dark matter leading to a transition between decelerating and accelerating phases of the Universe. This may challenge the Generalized Chaplygin Gas paradigm. However, in this paper we will show that the cosmic chronometers data do not favor the Dieterici proposal because of the tension between the estimates of the cosmological parameters when different redshift ranges of the cosmic history of the universe are considered, and because the model would be affected by a Big Rip singularity. Our analysis relies on a Bayesian Machine Learning technique which allows us to place tight constraints on our forecast.