  While a scalar field with a pole in its kinetic term is often used to study
the cosmological inflation, it can also play the role of dark energy, which is
called the pole dark energy model. We propose a generalized model that the
scalar field may have two or even multiple poles in the kinetic term and we
call it the multi-pole dark energy. We find the poles can place some
restrictions on the values of the original scalar field with non-canonical
kinetic term. After transforming to the canonical form, we get a flat potential
for the transformed new scalar field even if the original field has a steep
one. It The late-time evolution of the universe is obtained explicitly for the
two pole model, while dynamical analysis is performed for the multiple pole
model. We find that it does have a stable attractor solution, which corresponds
to the universe dominated by the potential of the scalar field.
