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Despite the nice features of the Dvali, Gabadadze and Porrati (DGP) model to explain the late-time acceleration of the universe, it suffers from some theoretical problems like the ghost issue.
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M. Bouhmadi-López and D. Wands, Phys. Rev. D 71
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V. Faraoni and S. Nadeau, Phys. Rev. D 72
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S. Nojiri and S. D. Odintsov, eConf C0602061
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R. Durrer and R. Maartens, arXiv:0811.4132 [astro-ph]
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K. Koyama, Class. Quant. Grav. 24
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S. Capozziello and M. Francaviglia, Gen. Rel. Grav. 40
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