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In this paper, we will present a Dvali-Gabadadze-Porrati stable model inorder to perform an observational test using $H(z)$ data and radial BAO scalein the galaxy distribution. In this vein, we study the tension betweenconstraints on the cosmological constant $\Lambda$ and the crossover scale$r_c$, which is associated with the DGP model. Our results show thatobservations do not favor the DGP stable model as a possible candidate to fitthe observations of the late cosmic acceleration.

Cosmological analysis of a DGP stable model with $H(z)$ observations a revision