  In this paper, we investigate some characteristics of phantom
Reissner-Nordstr\"om-de Sitter (RN-dS) black holes. The peculiar feature of
phantom field renders this kind of black holes quite different from their
counterparts. We can only find at most two horizons in this spacetime, i.e.
event horizon and cosmological horizon. For the black hole charge parameter, we
find that it is not bounded from below. We calculate quasinormal modes (QNMs)
frequencies of massless neutral scalar field perturbation in this black hole
spacetime, and some properties related to the large charge parameter are
disclosed.
