2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/217955In this article we have studied a closed universe which a holographic energy on the brane whose energy density is described by $ρ(H) =3c^{2}H^{2}$ and we obtain an equation for the Hubble parameter, this equation gave us different physical behavior depending if $c^2>1$ or $c^2<1$ against of the sign of the brane tension.General Relativity and Quantum Cosmologytext