Integral equation(Redirected from Integral equations)
The most basic type of integral equation is called a Fredholm equation of the first type,
The notation follows Arfken. Here φ is an unknown function, f is a known function, and K is another known function of two variables, often called the kernel function. Note that the limits of integration are constant: this is what characterizes a Fredholm equation.
If the unknown function occurs both inside and outside of the integral, the equation is known as a Fredholm equation of the second type,
If one limit of integration is a variable, the equation is called a Volterra equation. The following are called Volterra equations of the first and second types, respectively,
In all of the above, if the known function f is identically zero, the equation is called a homogeneous integral equation. If f is nonzero, it is called an inhomogeneous integral equation.
It is worth noting that integral equations often do not have an analytical solution, and must be solved numerically. An example of this is evaluating the Electric-Field Integral Equation (EFIE) or Magnetic-Field Integral Equation (MFIE) over an arbitrarily shaped object in an electromagnetic scattering problem.
One method to solve numerically requires discretizing variables and replacing integral by a quadrature rule
Then we have a system with n equations and n variables. By solving it we get the value of the n variables
Integral equations are classified according to three different dichotomies, creating eight different kinds:
- Limits of integration
- Placement of unknown function
- only inside integral: first kind
- both inside and outside integral: second kind
- Nature of known function f
- identically zero: homogeneous
- not identically zero: inhomogeneous
Integral equations are important in many applications. Problems in which integral equations are encountered include radiative transfer, and the oscillation of a string, membrane, or axle. Oscillation problems may also be solved as differential equations.
Both Fredholm and Volterra equations are linear integral equations, due to the linear behaviour of φ(x) under the integral. A nonlinear Volterra integral equation has the general form:
where F is a known function.
Wiener–Hopf integral equationsEdit
Originally, such equations were studied in connection with problems in radiative transfer, and more recently, they have been related to the solution of boundary integral equations for planar problems in which the boundary is only piecewise smooth.
Power series solution for integral equationsEdit
In many cases, if the Kernel of the integral equation is of the form K(xt) and the Mellin transform of K(t) exists, we can find the solution of the integral equation
in the form of a power series
are the Z-transform of the function g(s), and M(n + 1) is the Mellin transform of the Kernel.
Integral equations as a generalization of eigenvalue equationsEdit
where M = [Mi,j] is a matrix, v is one of its eigenvectors, and λ is the associated eigenvalue.
Taking the continuum limit, i.e., replacing the discrete indices i and j with continuous variables x and y, yields
where the sum over j has been replaced by an integral over y and the matrix M and the vector v have been replaced by the kernel K(x, y) and the eigenfunction φ(y). (The limits on the integral are fixed, analogously to the limits on the sum over j.) This gives a linear homogeneous Fredholm equation of the second type.
In general, K(x, y) can be a distribution, rather than a function in the strict sense. If the distribution K has support only at the point x = y, then the integral equation reduces to a differential eigenfunction equation.
In general, Volterra and Fredholm integral equations can arise from a single differential equation, depending on which sort of conditions are applied at the boundary of the domain of its solution.
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