  The recent observation of the cosmic microwave background anisotropy by the
WMAP confirmed that the lower multipoles are considerably suppressed. From the
standpoint of the cosmic variance, it is nothing but a statistical accident.
Alternatively, one can attribute the deficit of fluctuation on the large scale
to the cosmic history, which might be explained in the context of the
inflationary physics. In this paper, we show that it is possible to explain the
suppressed lower multipoles in the hybrid new inflation model.
