In mathematics, the inverse scattering transform is a method that solves the initial value problem for a nonlinear partial differential equation using mathematical methods related to wave scattering. The direct scattering transform describes how a function scatters waves or generates bound-states. The inverse scattering transform uses wave scattering data to construct the function responsible for wave scattering. The direct and inverse scattering transforms are analogous to the direct and inverse Fourier transforms which are used to solve linear partial differential equations.
Using a pair of differential operators, a 3-step algorithm may solve nonlinear differential equations; the initial solution is transformed to scattering data (direct scattering transform), the scattering data evolves forward in time (time evolution), and the scattering data reconstructs the solution forward in time (inverse scattering transform).
This algorithm simplifies solving a nonlinear partial differential equation to solving 2 linear ordinary differential equations and an ordinary integral equation, a method ultimately leading to analytic solutions for many otherwise difficult to solve nonlinear partial differential equations. The inverse scattering problem is equivalent to a Riemann–Hilbert factorization problem, at least in the case of equations of one space dimension. This formulation can be generalized to differential operators of order greater than two and also to periodic problems. In higher space dimensions one has instead a "nonlocal" Riemann–Hilbert factorization problem (with convolution instead of multiplication) or a d-bar problem.
The inverse scattering transform arose from studying solitary waves. J.S. Russell described a "wave of translation" or "solitary wave" occurring in shallow water. First J.V. Boussinesq and later D. Korteweg and G. deVries discovered the Korteweg-deVries (KdV) equation, a nonlinear partial differential equation describing these waves. Later, N. Zabusky and M. Kruskal, using numerical methods for investigating the Fermi–Pasta–Ulam–Tsingou problem, found that solitary waves had the elastic properties of colliding particles; the waves' initial and ultimate amplitudes and velocities remained unchanged after wave collisions. These particle-like waves are called solitons and arise in nonlinear equations because of a weak balance between dispersive and nonlinear effects.
Gardner, Greene, Kruskal and Miura introduced the inverse scattering transform for solving the Korteweg–de Vries equation. Lax, Ablowitz, Kaup, Newell, and Segur generalized this approach which led to solving other nonlinear equations including the nonlinear Schrödinger equation, sine-Gordon equation, modified Korteweg–De Vries equation, Kadomtsev–Petviashvili equation, the Ishimori equation, Toda lattice equation, and the Dym equation. This approach has also been applied to different types of nonlinear equations including differential-difference, partial difference, multidimensional equations and fractional integrable nonlinear systems.
The independent variables are a spatial variable
x
t
u(x,t)
The differential equation's solution meets the integrability and Fadeev conditions:
Integrability condition:
infty | |
\int | |
-infty |
|u(x)| dx <infty
Fadeev condition:
infty | |
\int | |
-infty |
(1+|x|))|u(x)| dx <infty
The Lax differential operators, and , are linear ordinary differential operators with coefficients that may contain the function or its derivatives. The self-adjoint operator has a time derivative and generates a eigenvalue (spectral) equation with eigenfunctions and time-constant eigenvalues (spectral parameters) .
L(\psi)=λ\psi,
\widetilde{\psi}=\psit-M(\psi)
(Lt+LM-ML)\psi=0
Lt+LM-ML=ut+N(u)=0
The direct scattering transform generates initial scattering data; this may include the reflection coefficients, transmission coefficient, eigenvalue data, and normalization constants of the eigenfunction solutions for this differential equation.
L(\psi)=λ\psi
The equations describing how scattering data evolves over time occur as solutions to a 1st order linear ordinary differential equation with respect to time. Using varying approaches, this first order linear differential equation may arise from the linear differential operators (Lax pair, AKNS pair), a combination of the linear differential operators and the nonlinear differential equation, or through additional substitution, integration or differentiation operations. Spatially asymptotic equations () simplify solving these differential equations.
The Marchenko equation combines the scattering data into a linear Fredholm integral equation. The solution to this integral equation leads to the solution, u(x,t), of the nonlinear differential equation.
The nonlinear differential Korteweg–De Vries equation is
ut-6uux+uxxx=0
The Lax operators are:
L=
2 | |
-\partial | |
x |
+u(x,t)
Lt+LM-ML=ut-6uux+uxxx=0
The solutions to this differential equation
may include scattering solutions with a continuous range of eigenvalues (continuous spectrum) and bound-state solutions with discrete eigenvalues (discrete spectrum). The scattering data includes transmission coefficients , left reflection coefficient , right reflection coefficient , discrete eigenvalues , and left and right bound-state normalization (norming) constants.
c(0)Lj=\left(
infty | |
\int | |
-infty |
2 | |
\psi | |
L |
(ikj,x,0) dx\right)-1/2 j=1,...,N
c(0)Rj=\left(
infty | |
\int | |
-infty |
2 | |
\psi | |
R |
(ikj,x,0) dx\right)-1/2 j=1,...,N
The spatially asymptotic left and right Jost functions simplify this step.
\begin{align} \psiL(x,k,t)&=eikx+o(1), x\to+infty\\ \psiL(x,k,t)&=
eikx | + | |
T(k,t) |
RL(k,t)e-ikx | |
T(k,t) |
+o(1), x\to-infty\ \psiR(x,k,t)&=
e-ikx | + | |
T(k,t) |
RR(k,t)eikx | |
T(k,t) |
+o(1), x\to+infty\ \psiR(x,k,t)&=e-ikx+o(1), x\to-infty\\ \end{align}
\gammaj(t)=
\psiL(x,i\kappaj,t) | |
\psiR(x,i\kappaj,t) |
=(-1)N-j
cRj(t) | |
cLj(t) |
\partialt\psiL(k,x,t)-M\psiL(x,k,t)=aL(k,t)\psiL(x,k,t)+bL(k,t)\psiR(x,k,t)
\partialt\psiR(k,x,t)-M\psiR(x,k,t)=aR(k,t)\psiL(x,k,t)+bR(k,t)\psiR(x,k,t)
\begin{align}RL(k,t)&=RL
-i8k3t | |
(k,0)e |
\\ RR(k,t)&=RR
+i8k3t | |
(k,0)e |
\ cLj(t)&=cLj
| ||||||||||
(0)e |
, j=1,\ldots,N\\ cRj(t)&=cRj
| ||||||||||
(0)e |
, j=1,\ldots,N\end{align}
The Marchenko kernel is .
F(x,t)\overset{def}{=} | 1 |
2\pi |
infty | |
\int | |
-infty |
RR(k,t) eikx dk+
N | |
\sum | |
j=1 |
2 | |
c(t) | |
Lj |
-\kappajx | |
e |
The Marchenko integral equation is a linear integral equation solved for .
K(x,z,t)+F(x+z,t)+
infty | |
\int | |
x |
K(x,y,t)F(y+z,t) dy=0
The solution to the Marchenko equation, , generates the solution to the nonlinear partial differential equation.
u(x,t)=-2
\partialK(x,x,t) | |
\partialx |