We present an approximate analysis of a nonlinear effect of parametric osci
llatory instability in Fabry-Perot (FP) interferometer. The basis for this
effect is the excitation of the additional (Stokes) optical mode with frequ
ency omega (1) and of the mirror's elastic mode with frequency omega (m), w
hen the optical energy stored in the FP resonator main mode with frequency
omega (0) exceeds the certain threshold and the frequencies are related as
omega (0) similar or equal to, omega (1) + omega (m). This effect is undesi
rable in laser gravitational wave antennae because it may create a specific
upper limit for the value of energy stored in FP resonator. In order to av
oid it the detailed analysis of the mirror's elastic modes and FP resonator
optical modes structure is necessary. (C) 2001 Published by Elsevier Scien
ce B.V.