It appears difficult to construct a simple model for an open universe based
on the one bubble inflationary scenario. The reason is that one needs a la
rge mass to avoid the tunneling via the Hawking-Moss solution and a small m
ass for successful slow-rolling. However, Rubakov and Sibiryakov suggest th
at the Hawking-Moss solution is not a solution for the false vacuum decay p
rocess because it does not satisfy the boundary condition. Hence, we have r
econsidered the arguments for the defect of the simple polynomial model. We
point out the possibility that one of the valley bounce belonging to a val
ley line in the functional space represents the decay process instead of th
e Hawking-Moss solution. Under this presumption, we show an open inflation
model can be constructed within the polynomial form of the potential so tha
t the fluctuations can be reconciled with the observations. (C) 2000 Elsevi
er Science B.V. All rights reserved.