  Basing on the ideas used by Kiselev, we study three black holes surrounded by
quintessence and the effects of quintessence on the classical and semiclassical
scattering cross-sections. In contrast, the absorption section is studied with
the sinc approximation in the eikonal limit. For Schwarzschild,
Reissner-Nordstr\"{o}m and Bardeen black holes surrounded by quintessence, the
values critical of charges and the normalization factor are obtained. We also
described the horizons and the extremal condition of the black holes surrounded
by quintessence. By setting for the quintessence state parameter in two the
particular cases w=-2/3 and w=-1/2.
