  The Lorentz symmetry of gravity is spontaneously broken when the nonminimally
coupled Kalb-Ramond field acquires a nonzero vacuum expectation value. In this
work, we present exact solutions for static and spherically symmetric black
holes in the framework of this Lorentz-violating gravity theory. In order to
explore the physical implications of Lorentz violation, we analyze the
thermodynamic properties of the obtained solutions and evaluate the impact of
Lorentz violation on some classical gravitational experiments within the Solar
System. Furthermore, the Lorentz-violating parameter is constrained by using
the measured results of these experiments.
