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In this work, we will analyze a noncommutative (NC) phase space version of the Friedmann–Robert–Walker cosmological models within the gravitational Hořava–Lifshitz theory. The matter content of the models is described by a perfect fluid and the constant curvature of the spatial sections may be positive, negative or zero. In order to obtain this theory, we will use the Faddeev–Jackiw symplectic formalism...
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