We show that the potential of the scalar field in the Einstein frame is flat
if the nonminimal coupling term is properly chosen that it satisfies the
condition (V(phi)/K^2(phi)-> constant) as phi gets large. The cosmological
implication of this theory is studied.Comment: Talk at the international Workshop on e-Science for Physics 2008
during September 8-9, 2008 at Daejeon Convention Center, Daejeon, Kore