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Differential and Integral Equation




                    Notes          11.4 Bessel’s Inequality, Approximation in the Mean and
                                       Completeness


                                   We can now define a sequence of orthonormal eigenfunctions
                                                           y
                                                             x
                                                        r ( ) ( ,  n )
                                                         x
                                             x
                                            ( )
                                           n
                                                     y
                                                  r ( ) ( ,  n ), r ( ) ( ,  n )
                                                    x
                                                                y
                                                                  x
                                                       x
                                                               x
                                   which satisfy
                                             x
                                             ( ),  ( )  nm ,                                              ...(13)
                                                  x
                                            n    m
                                   where    is the Kronecker delta. We will try  to  establish  when we can  write a  piecewise
                                         nm
                                   continuous function f(x) in the form
                                                
                                            x
                                                     x
                                          f ( )   a f ( )                                                 ...(14)
                                                   i i
                                               i  0
                                   Taking the inner product of both sides of this series with  (x) shows that
                                                                                  j
                                          a  j  f ( ),  j ( ) ,                                           ...(15)
                                                     x
                                                x
                                   using the orthonormality condition (13). The quantities a  are known as the expansion coefficients,
                                                                               i
                                   or generalized Fourier coefficients. In order to motivate the infinite series expansion (14), we
                                   start by approximating f(x) by a finite sum,
                                                 Ν
                                             x
                                                      x
                                          f  ( )   A f ( ,  )
                                           N        i    i
                                                i  0
                                   for some finite N, where the  A are to be determined so that this provides the most accurate
                                                            i
                                   approximation to f(x). The error in this approximation is
                                                      Ν
                                                           x
                                             x
                                          R N ( )  f ( )  A f ( ,  i )
                                                  x
                                                          i
                                                      i  0
                                   We now try to minimize this error by minimizing its norm
                                                                              2
                                                               b      Ν
                                              2
                                                                           x
                                                         x
                                                                  x
                                                    x
                                           R N   R N ( ), R N ( )  f ( )  A f ( ) dx ,
                                                                         i i
                                                              a
                                                                     i  0
                                   which is the mean square error in the approximation. Now
                                                       Ν             Ν
                                              2
                                                             x
                                                               f
                                                   x
                                                                 x
                                                                          x
                                           R N    f ( )  A f  ( ), ( )  A f ( )
                                                          i i
                                                                        i i
                                                       i  0         i  0
                                                            Ν
                                                    2
                                                  x
                                                         x
                                                f  ( )  f ( ),  A f ( )
                                                                  x
                                                                i i
                                                            i  0
                                             Ν               Ν       Ν
                                                                  x
                                                     f
                                               A f ( ), ( )    A f ( ),  A f  ( )
                                                   x
                                                       x
                                                                           x
                                                                        i i
                                                i i
                                                                i i
                                            i  0            i  0     i  0
                                   We can now use the orthonormality of the eigenfunctions (13) and the expression (15), which
                                   determines the coefficients a , to obtain
                                                          i
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