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We present an holographic model of the Dvali-Gabadadze-Porrati scenario with a Gauss-Bonnet term in the bulk.
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There are alternative approaches to explain the current observational data based on dropping the asumption of homogeneity and/or isotropy of the (“background”) universe. See [ 6 ] and references therein for details
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We refer the readers as well to [ 12 ] , where the holographic bound on entropy was first considered. We thank González-Díaz for pointing out this to us
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