In this work, we investigate the scattering of a massless scalar wave by a
Schwarzschild black hole in gravity modified by a background Kalb-Ramond field,
which induces spontaneous Lorentz symmetry violation. The Klein-Gordon equation in
this background is solved analytically, and the radial part of the wave equation is
expressed in terms of confluent Heun functions. By analyzing the near-horizon
behavior of the scalar field, we derive the Hawking radiation spectrum and
demonstrate that Lorentz-violating effects enhance the effective temperature and the
emitted energy flux. In the asymptotic region, we show that the radial equation
reduces to a Coulomb-like form, allowing us to obtain closed-form expressions for the
phase shifts. It is shown that Lorentz symmetry violation significantly modifies both
the frequency dependence and the angular distribution of the scattered scalar waves.
In addition, we obtain the quasinormal mode spectrum under appropriate boundary
conditions and discuss its implications for the stability of the Lorentz-violating black
hole solution. Our analysis suggests that scalar-wave dynamics around black holes
provides a sensitive probe to test Lorentz-violating effects.