• Source: Three-wave equation
    • In nonlinear systems, the three-wave equations, sometimes called the three-wave resonant interaction equations or triad resonances, describe small-amplitude waves in a variety of non-linear media, including electrical circuits and non-linear optics. They are a set of completely integrable nonlinear partial differential equations. Because they provide the simplest, most direct example of a resonant interaction, have broad applicability in the sciences, and are completely integrable, they have been intensively studied since the 1970s.


      Informal introduction


      The three-wave equation arises by consideration of some of the simplest imaginable non-linear systems. Linear differential systems have the generic form




      D
      ψ
      =
      λ
      ψ


      {\displaystyle D\psi =\lambda \psi }


      for some differential operator D. The simplest non-linear extension of this is to write




      D
      ψ

      λ
      ψ
      =
      ε

      ψ

      2


      .


      {\displaystyle D\psi -\lambda \psi =\varepsilon \psi ^{2}.}


      How can one solve this? Several approaches are available. In a few exceptional cases, there might be known exact solutions to equations of this form. In general, these are found in some ad hoc fashion after applying some ansatz. A second approach is to assume that



      ε

      1


      {\displaystyle \varepsilon \ll 1}

      and use perturbation theory to find "corrections" to the linearized theory. A third approach is to apply techniques from scattering matrix (S-matrix) theory.
      In the S-matrix approach, one considers particles or plane waves coming in from infinity, interacting, and then moving out to infinity. Counting from zero, the zero-particle case corresponds to the vacuum, consisting entirely of the background. The one-particle case is a wave that comes in from the distant past and then disappears into thin air; this can happen when the background is absorbing, deadening or dissipative. Alternately, a wave appears out of thin air and moves away. This occurs when the background is unstable and generates waves: one says that the system "radiates". The two-particle case consists of a particle coming in, and then going out. This is appropriate when the background is non-uniform: for example, an acoustic plane wave comes in, scatters from an enemy submarine, and then moves out to infinity; by careful analysis of the outgoing wave, characteristics of the spatial inhomogeneity can be deduced. There are two more possibilities: pair creation and pair annihilation. In this case, a pair of waves is created "out of thin air" (by interacting with some background), or disappear into thin air.
      Next on this count is the three-particle interaction. It is unique, in that it does not require any interacting background or vacuum, nor is it "boring" in the sense of a non-interacting plane-wave in a homogeneous background. Writing




      ψ

      1


      ,

      ψ

      2


      ,

      ψ

      3




      {\displaystyle \psi _{1},\psi _{2},\psi _{3}}

      for these three waves moving from/to infinity, this simplest quadratic interaction takes the form of




      (
      D

      λ
      )

      ψ

      1


      =
      ε

      ψ

      2



      ψ

      3




      {\displaystyle (D-\lambda )\psi _{1}=\varepsilon \psi _{2}\psi _{3}}


      and cyclic permutations thereof. This generic form can be called the three-wave equation; a specific form is presented below. A key point is that all quadratic resonant interactions can be written in this form (given appropriate assumptions). For time-varying systems where



      λ


      {\displaystyle \lambda }

      can be interpreted as energy, one may write




      (
      D

      i


      /


      t
      )

      ψ

      1


      =
      ε

      ψ

      2



      ψ

      3




      {\displaystyle (D-i\partial /\partial t)\psi _{1}=\varepsilon \psi _{2}\psi _{3}}


      for a time-dependent version.


      Review


      Formally, the three-wave equation is









      B

      j





      t



      +

      v

      j





      B

      j


      =

      η

      j



      B








      B

      m







      {\displaystyle {\frac {\partial B_{j}}{\partial t}}+v_{j}\cdot \nabla B_{j}=\eta _{j}B_{\ell }^{*}B_{m}^{*}}


      where



      j
      ,

      ,
      m
      =
      1
      ,
      2
      ,
      3


      {\displaystyle j,\ell ,m=1,2,3}

      cyclic,




      v

      j




      {\displaystyle v_{j}}

      is the group velocity for the wave having







      k





      j


      ,

      ω

      j




      {\displaystyle {\vec {k}}_{j},\omega _{j}}

      as the wave-vector and angular frequency, and






      {\displaystyle \nabla }

      the gradient, taken in flat Euclidean space in n dimensions. The




      η

      j




      {\displaystyle \eta _{j}}

      are the interaction coefficients; by rescaling the wave, they can be taken




      η

      j


      =
      ±
      1


      {\displaystyle \eta _{j}=\pm 1}

      . By cyclic permutation, there are four classes of solutions. Writing



      η
      =

      η

      1



      η

      2



      η

      3




      {\displaystyle \eta =\eta _{1}\eta _{2}\eta _{3}}

      one has



      η
      =
      ±
      1


      {\displaystyle \eta =\pm 1}

      . The



      η
      =

      1


      {\displaystyle \eta =-1}

      are all equivalent under permutation. In 1+1 dimensions, there are three distinct



      η
      =
      +
      1


      {\displaystyle \eta =+1}

      solutions: the



      +
      +
      +


      {\displaystyle +++}

      solutions, termed explosive; the





      +


      {\displaystyle --+}

      cases, termed stimulated backscatter, and the




      +



      {\displaystyle -+-}

      case, termed soliton exchange. These correspond to very distinct physical processes. One interesting solution is termed the simulton, it consists of three comoving solitons, moving at a velocity v that differs from any of the three group velocities




      v

      1


      ,

      v

      2


      ,

      v

      3




      {\displaystyle v_{1},v_{2},v_{3}}

      . This solution has a possible relationship to the "three sisters" observed in rogue waves, even though deep water does not have a three-wave resonant interaction.
      The lecture notes by Harvey Segur provide an introduction.
      The equations have a Lax pair, and are thus completely integrable. The Lax pair is a 3x3 matrix pair, to which the inverse scattering method can be applied, using techniques by Fokas. The class of spatially uniform solutions are known, these are given by Weierstrass elliptic ℘-function. The resonant interaction relations are in this case called the Manley–Rowe relations; the invariants that they describe are easily related to the modular invariants




      g

      2




      {\displaystyle g_{2}}

      and




      g

      3


      .


      {\displaystyle g_{3}.}


      That these appear is perhaps not entirely surprising, as there is a simple intuitive argument. Subtracting one wave-vector from the other two, one is left with two vectors that generate a period lattice. All possible relative positions of two vectors are given by Klein's j-invariant, thus one should expect solutions to be characterized by this.
      A variety of exact solutions for various boundary conditions are known. A "nearly general solution" to the full non-linear PDE for the three-wave equation has recently been given. It is expressed in terms of five functions that can be freely chosen, and a Laurent series for the sixth parameter.


      Applications


      Some selected applications of the three-wave equations include:

      In non-linear optics, tunable lasers covering a broad frequency spectrum can be created by parametric three-wave mixing in quadratic (




      χ

      (
      2
      )




      {\displaystyle \chi ^{(2)}}

      ) nonlinear crystals.
      Surface acoustic waves and in electronic parametric amplifiers.
      Deep water waves do not in themselves have a three-wave interaction; however, this is evaded in multiple scenarios:
      Deep-water capillary waves are described by the three-wave equation.
      Acoustic waves couple to deep-water waves in a three-wave interaction,
      Vorticity waves couple in a triad.
      A uniform current (necessarily spatially inhomogenous by depth) has triad interactions.
      These cases are all naturally described by the three-wave equation.
      In plasma physics, the three-wave equation describes coupling in plasmas.


      References

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