Spherically symmetric, static black holes with scalar hair, and naked singularities in nonminimally coupled k-essence

We apply a recently developed 2 + 1 + 1 decomposition of spacetime, based on a nonorthogonal double foliation for the study of spherically symmetric, static black hole solutions of Horndeski scalar-tensor theory. Our discussion proceeds in an effective field theory (EFT) of modified gravity approach, with the action depending on metric and embedding scalars adapted to the nonorthogonal 2 + 1 + 1 decomposition. We prove that the most generic class of Horndeski Lagrangians compatible with observations can be expressed in this EFT form. By studying the first order perturbation of the EFT action we derive three equations of motion, which reduce to those derived earlier in an orthogonal 2 + 1 + 1 decomposition, and a fourth equation for the metric parameter Ar related to the nonorthogonality of the foliation. For the Horndeski class of theories with vanishing G(3) and G(5), but generic functions G(2) (phi, X) (k-essence) and G(4)(phi) (nonminimal coupling to the metric) we prove the unicity theorem that no action beyond EinsteinHilbert allows for the Schwarzschild solution. Next we integrate the EFT field equations for the case with only one independent metric function, and we obtain new solutions characterized by a parameter, which in the simplest cases has the interpretation of mass or tidal charge, the cosmological constant and a third parameter. These solutions represent naked singularities, black holes with scalar hair or have the double horizon structure of the Schwarzschild-de Sitter spacetime. Solutions with homogeneous Kantowski-Sachs type regions also emerge. Finally, one of the solutions obtained for the function G(4) linear in the curvature coordinate, in certain parameter range exhibits an intriguing logarithmic singularity lying outside the horizon. The newly derived hairy black hole solutions evade previously known unicity theorems by being asymptotically nonflat, even in the absence of the cosmological constant.