  We have studied quasinormal modes of spinor $\frac{1}{2}$, massless Dirac
field perturbations of a black hole in massive gravity. The parameters of the
theory, such as the mass of the black hole, the scalar charge of the black
hole, mode number and the multipole number are varied to observe how the
corresponding quasinormal frequencies change. We have also used the
P$\ddot{o}$schl-Teller approximation to reach analytical values for the
frequencies of quasinormal modes for comparison with the numerically obtained
values. Comparisons are done with the frequencies of the Schwarzschild black
hole.
