We study quasi-nonlinear evolution of the density perturbation in Newt
onian gravity. Weak mode-mode coupling in a small range below the Jean
s wavelength is considered. In order to extract nonlinear dynamics we
utilize a reductive perturbation, which is well known in mechanics and
hydrodynamics and improves a naive perturbation. We show that the bas
ic equations for the acoustic wave reduce to a nonlinear Schrodinger e
quation. It describes a competition between dispersion originated from
gravitational attraction and nonlinearity up to cubic order of the am
plitude of the acoustic wave. In purely 1-dimensional motion, there ex
ists localized structures as soliton solutions of two distinctive type
s depending on the wavelength. More interesting is an instability pres
ent in 3-dimensional motion. Namely, a progressive wave is unstable un
der a long-wave perturbation transverse to the direction of progressio
n. It may imply a possible nonlinear growth of the density fluctuation
below the Jeans scale.