Modulational instability

In the fields of nonlinear optics and fluid dynamics, modulational instability or sideband instability is a phenomenon whereby deviations from a periodic waveform are reinforced by nonlinearity, leading to the generation of spectral-sidebands and the eventual breakup of the waveform into a train of pulses. In the fields of nonlinear optics and fluid dynamics, modulational instability or sideband instability is a phenomenon whereby deviations from a periodic waveform are reinforced by nonlinearity, leading to the generation of spectral-sidebands and the eventual breakup of the waveform into a train of pulses. The phenomenon was first discovered − and modelled − for periodic surface gravity waves (Stokes waves) on deep water by T. Brooke Benjamin and Jim E. Feir, in 1967. Therefore, it is also known as the Benjamin−Feir instability. It is a possible mechanism for the generation of rogue waves. Modulation instability only happens under certain circumstances. The most important condition is anomalous group velocity dispersion, whereby pulses with shorter wavelengths travel with higher group velocity than pulses with longer wavelength. (This condition assumes a focussing Kerr nonlinearity, whereby refractive index increases with optical intensity.) The instability is strongly dependent on the frequency of the perturbation. At certain frequencies, a perturbation will have little effect, whilst at other frequencies, a perturbation will grow exponentially. The overall gain spectrum can be derived analytically, as is shown below. Random perturbations will generally contain a broad range of frequency components, and so will cause the generation of spectral sidebands which reflect the underlying gain spectrum. The tendency of a perturbing signal to grow makes modulation instability a form of amplification. By tuning an input signal to a peak of the gain spectrum, it is possible to create an optical amplifier. The gain spectrum can be derived by starting with a model of modulation instability based upon the nonlinear Schrödinger equation which describes the evolution of a complex-valued slowly varying envelope A {displaystyle A} with time t {displaystyle t} and distance of propagation z {displaystyle z} . The imaginary unit i {displaystyle i} satisfies i 2 = − 1. {displaystyle i^{2}=-1.} The model includes group velocity dispersion described by the parameter β 2 {displaystyle eta _{2}} , and Kerr nonlinearity with magnitude γ . {displaystyle gamma .} A periodic waveform of constant power P {displaystyle P} is assumed. This is given by the solution where the oscillatory e i γ P z {displaystyle e^{igamma Pz}} phase factor accounts for the difference between the linear refractive index, and the modified refractive index, as raised by the Kerr effect. The beginning of instability can be investigated by perturbing this solution as where ε ( t , z ) {displaystyle varepsilon (t,z)} is the perturbation term (which, for mathematical convenience, has been multiplied by the same phase factor as A {displaystyle A} ). Substituting this back into the nonlinear Schrödinger equation gives a perturbation equation of the form