Buildup times and the stationary values of spin wave excitations near the S
uhl instability threshold are calculated numerically. The study is done in
the framework of the two-mode model. The time evolution of the excitation m
ay approach the steady state via oscillations that may last for a very long
time. The stationary excitation N-0, and the buildup time tau(b) depend on
the pumping power p, and the pumping field h via power laws: N-0 = B(p/p(c
) - 1)(delta) and tau(b) = A(h/h(c) - 1)(-Delta). For the case of no de-tun
ing of the mode frequencies from omega(p)/2, delta = 0.5 and Delta = 0.98.
In the case of modes that are de-tuned from omega(p)/2, delta = 0.42 and De
lta = 1.1. The values for delta are consistent with experiments but the val
ues for delta are in bad agreement with experiment. It is shown that if a f
inite medium correction term is introduced into the equations of motion the
threshold of the pumping field amplitude is below gamma/V where gamma is t
he spin wave relaxation rate and V is the coupling of the spin waves to the
pumping field. This result is very strange and raises serious doubts about
the justification of the finite medium correction term. (C) 1999 Published
by Elsevier Science B.V. All rights reserved.