  We compute the quasinormal frequencies for scalar perturbations of charged
black holes in five-dimensional Einstein-power-Maxwell theory. The impact on
the spectrum of the electric charge of the black holes, of the angular degree,
of the overtone number, and of the mass of the test scalar field is
investigated in detail. The quasinormal spectra in the eikonal limit are
computed as well for several different space-time dimensionalities.
