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تسجيل مستخدم جديدHolographic Cosmological Models on the Braneworld
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In this article we have studied a closed universe which a holographic energy on the brane whose energy density is described by $rho (H) =3c^{2}H^{2}$ 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.
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