“…Indeed in this manifold, the Riemann tensor is a function of the Ricci tensor and metric R αβγσ (R µν , g µν ), them if we consider the Einstein-Hilbert action there is no solutions, nevertheless, when a negative cosmological constant is considered Banados, Teitelboim and Zanelli found the BTZ black hole solution [3,4]. The procedure to overcome the non-hair theorem consist in coupling (minimal, non-minimal or conformal) another fields to Einstein-Hilbert, but under the special conditions [2,[5][6][7][8][9][10], And no less important is the route of higherderivative gravities [11][12][13], another examples with scalar hair and gauge fields in fourth dimensions can be found in [14][15][16][17][18][19][20] Here we present a family of hairy black hole solutions in three dimensions with a non-trivial scalar potential minimally coupling. This scalar field contributes to the metric, therefore, in to the thermodynamics of the black hole.…”