In this paper, using the maximal embedding of into in the Euler angles parameterization, we construct a novel family of exact solutions of the Einstein -Skyrme model. First, we present a hairy toroidal black hole in dimensions. This solution is asymptotically locally anti-de Sitter and is characterized by discrete hair parameters. Then, we perform a dimensional extension of the black hole to obtain black -branes as solutions of the Einstein -Non-linear sigma model in dimensions. These are homogeneous and topologically protected. Finally we show that, through a Wick rotation of the toroidal black hole, one can construct an exact self-gravitating instanton. The role that the flavor number plays in the geometry and thermodynamics of these configurations is also discussed.

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