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11.9. The Carleman Method for Integral Equations of
                       Convolution Type of the Second Kind

                 11.9-1. The Wiener–Hopf Equation of the Second Kind

               Equations of convolution type of the second kind of the form*

                                       1    ∞
                                y(x)+ √       K(x – t)y(t) dt = f(x),  0 < x < ∞,           (1)
                                       2π  0
               frequently occur in applications. Here the domain of the kernel K(x) is the entire real axis.
                   Let us extend the equation domain to the negative semiaxis by introducing one-sided functions,

                            y(x)  for x >0,           f(x)  for x >0,
                   y + (x)=                   f + (x)=                   y – (x)=0  for x >0.
                            0    for x <0,            0     for x <0,
               Then we obtain an equation,

                                         ∞
                                   1
                          y + (x)+ √      K(x – t)y + (t) dt = y – (x)+ f + (x),  –∞ < x < ∞,  (2)
                                   2π  –∞
               which coincides with (1) for x >0.
                   The auxiliary function y – (x) is introduced to compensate for the left-hand side of Eq. (2) for
               x < 0. Note that y – (x) is unknown for x < 0 and is to be found in solving the problem.
                   Let us pass to the Fourier integrals in Eq. (2) (see Subsections 7.4-3, 10.4-1, and 10.4-2). We
               obtain a Riemann problem in the form

                                             –
                                                      +
                                           Y (u)     F (u)
                                    +
                                   Y (u)=         +        ,    –∞ < u < ∞.                 (3)
                                          1+ K(u)   1+ K(u)
                ◦
               1 . Assume that the normality condition is satisfied, i.e.,
                                                 1+ K(u) ≠ 0,
               then we rewrite the Riemann problem in the usual form

                                                –
                                     +
                                    Y (u)= D(u)Y (u)+ H(u),    –∞ < u < ∞,                  (4)
               where
                                                 1              F(u)
                                       D(u)=         ,  H(u)=         .                     (5)
                                              1+ K(u)          1+ K(u)
                   The Riemann problem (4) is equivalent to Eq. (1); in particular, these equations are simulta-
               neously solvable or unsolvable and have an equal number of arbitrary constants in their general
               solutions. If the index ν of the Riemann problem, which is given by the relation

                                                          1
                                                ν = Ind                                     (6)
                                                       1+ K(u)
               (which is also sometimes called the index of the Wiener–Hopf equation of the second kind), is
               positive, then the homogeneous equation (1) (f(x) ≡ 0) has exactly ν linearly independent solutions,
              * Prior to reading this section looking through Sections 10.4 and 10.5 is recommended.




                 © 1998 by CRC Press LLC








               © 1998 by CRC Press LLC
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