  In this paper, we investigate the influence of anti-symmetric tensor effects,
which trigger the Lorentz symmetry breaking, on charged spherically symmetric
black holes. Initially, we address an overview of the model, laying the
groundwork for deriving solutions to black holes. With this, we analyze the
horizons, critical orbits, and geodesics. We compute quasinormal modes with a
particular emphasis on vectorial perturbations. In addition, we derive the
Hawking temperature to perform the calculation of the remnant mass.
Additionally, we estimate the lifetime of the black holes until they reach
their final stage after the evaporation process. Furthermore, we explore the
emission rate, and the deflection angle. Finally, we investigate the
correlation between quasinormal modes and shadows.
