  The quasinormal modes of charged and uncharged massive scalar fields and also
of charged Dirac fields against the background of a charged spherical black
hole endowed with a scalar hair have been investigated. Special emphasis has
been given to the case where negative scalar charge dominates over the electric
charge of the black hole which mimics an Einstein-Rosen bridge. Except for the
complete monotonic behaviour of the damping (imaginary part of the quasinormal
mode) against the charge of the black hole as opposed to the existence of a
peak for the pure RN case, the qualitative behaviour does not appreciably
change due to the presence of scalar hair.
