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Expansion by orthogonal systems of functions in Hilbert space. Complete orthogonal systems. Orthonormal systems. Generalized Fourier series, coefficients. Parseval’s identity.




Def. Orthogonal system. A system of functions


             ole.gif


is called orthogonal if every function is orthogonal to every other function i.e. if


             ole1.gif



Examples of orthogonal systems.

 

1. The sequence of trigonometric functions

 

            1, cos x, sin x, cos 2x, sin 2x, .... , cos nx, sin nx, .....

 

on the interval (-π, π). This system is one of the first and most important examples of orthogonal systems, appearing in works of Euler, D. Bernoulli, and d’Alembert in connection with problems on oscillation of strings. The study of it has played an essential role in the development of analysis.

 

2. The sequence of Legendre polynomials

 

             ole2.gif  

 

on the interval (-1, 1). The first few polynomials of the sequence are

 

             ole3.gif

 

 

Def. Orthonormal system. A system of functions

 

             ole4.gif

 

is called orthonormal if it is orthogonal and if each of the functions is of unit length i.e.

 

             ole5.gif                                                                                                                                                              

 

Example. The sequence of trigonometric functions

 

             ole6.gif

 

on the interval (-π, π) is orthonormal. These functions are obtained by dividing the functions

 

            1, cos x, sin x, cos 2x, sin 2x, .... , cos nx, sin nx, .....

 

by their lengths.

ole7.gif

 

 

Expansion by orthogonal systems of functions. Let e1 and e2 be any two mutually perpendicular vectors of unit length in the plane. See Fig. 1. Then any vector f in the plane can decomposed in the direction of these two vectors and written as

 

            f = a1e1 + a2e2

 

ole8.gif

where a1 = f•e1 and a2 = f•e2 as shown in Fig. 2. Similarly if e1, e2 and e3 are any three mutually perpendicular unit vectors in three-dimensional space any vector f in space can be decomposed in the direction of these three vectors and written as

 

            f = a1e1 + a2e2 + a3e3

 

where a1 = f•e1, a2 = f•e2 and a3 = f•e3 .

 

Just as it is possible to represent any vector f in three-dimensional space as a linear combination

 

            f = a1e1 + a2e2 + a3e3

 

of three pairwise orthogonal unit vectors it is possible to represent any function f in Hilbert space as a linear combination of an orthonormal system of functions. For this to be so, however, it is necessary for the orthonormal system to be complete.

 

Def. Complete orthogonal system. An orthogonal system of functions is called complete if it is impossible to add to it even one function, not identically equal to zero, that is orthogonal to all the functions of the system.

 

It is easy to give an example of an orthogonal system that is not complete. If we are given any arbitrary orthogonal system and remove a single function from it, the remaining system will be incomplete. Suppose, for example, that we remove cos x from orthogonal system

 

            1, cos x, sin x, cos 2x, sin 2x, .... , cos nx, sin nx, .....

 

The remaining system

 

            1, sin x, cos 2x, sin 2x, .... , cos nx, sin nx, .....

 

is orthogonal as before, but it is not complete since the function cos x which we excluded is orthogonal to all functions of the system.

 

 

Theorem 1. Let a complete orthonormal system of functions in Hilbert space

 

             ole9.gif

 

be given. Then every function f(x) in the space can be represented by a series

 

ole10.gif

 

where the coefficients an of the expansion are equal to the projections of the vector f on the elements of the normal orthogonal system i.e.

 

             ole11.gif

 

Because of the analogy with Fourier series 1) is sometimes called a generalized Fourier series and the coefficients an generalized Fourier coefficients.

 

The formula above for an is easily derived. If we multiply both sides of 1) scalarly by any function fn of the system, we get

 

ole12.gif

 

Because fmfn = 0 for m ≠ n and fnfn = 1, equation 2) reduces to

 

             ole13.gif

 

             

Theorem 2 (Parseval’s identity). The square of the length of a vector in Hilbert space is equal to the sum of the squares of its projections onto a complete system of mutually orthogonal directions. In other words, if

 

             ole14.gif

 

are a complete orthonormal system of functions in Hilbert space and if a function f is given by

 

             ole15.gif

 

then

 

ole16.gif

 

Proof

 

 

Condition of completeness. The condition of completeness for a functional space is that 3) hold for an arbitrary function of the space.

 

Analogue of the concept of completeness in n-dimensional space. In n-dimensional space any vector in the space can be expressed as a linear combination of n linearly independent basis vectors. However, not every vector in the space can be expressed as a linearly combination of only n-1 of the basis vectors. If one of the basis vectors is missing, not all vectors in the space can be expressed as a linear combination of the remaining basis vectors. The condition of completeness of an orthogonal system of functions corresponds to the requirement for a full set of n basis vectors for an n-dimensional space.

 

 

References

  Mathematics, Its Content, Methods and Meaning. Vol. 3, Chap. XIX



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