  We have studied quasinormal modes of scalar 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 and the spherical harmonic index is
varied to see how the corresponding quasinormal frequencies change. We have
also studied the massive scalar field perturbations. Most of the work is done
using WKB approach while sections are devoted to compute quasinormal modes via
the unstable null geodesics approach and the Poschl-Teller approximation.
Comparisons are done with the Schwarzschild black hole.
