We address the problem of classical frictional motion under a potentia
l V possessing a barrier, apart from other possible confining and nons
tationary terms. It is pointed out that the Green's solution of the ex
act equation of motion can be reduced (under suitable conditions) eith
er to an improved Rayleigh form or a non-Rayleigh form, the latter bei
ng outside the scope of the standard large-friction treatment of the F
okker-Planck equation. The resulting dissipationless dynamics involves
an appropriately scaled potential which may have promising applicatio
ns to quantum stochastic phenomena. Genuine dissipative corrections in
regions far away from the barrier can be accounted for by the higher-
order terms in our asymptotic expansions.