Static spherical vacuum solutions in the bumblebee gravity model

The bumblebee gravity model is a vector-tensor theory of gravitation where the vector field nonminimally couples to Ricci tensor. By investigating vacuum equations with spherical symmetry, we find two families black-hole (BH) solutions in this model: one has vanishing radial component and other When coupling between tensor set zero, first family becomes Reissner-Nordstr\"om solution while second degenerates Schwarzschild being zero. General numerical both are obtained for nonzero Besides BH solutions, also reveal existence that have nonvanishing $tt$-component metric on supposed event horizon $rr$-component diverges curvature scalars finite. These not supported by existing observations but present certain properties academic interests. We conclude study putting into tests against Solar-system images supermassive BHs.