Exponential sum

In mathematics, an exponential sum may be a finite Fourier series (i.e. a trigonometric polynomial), or other finite sum formed using the exponential function, usually expressed by means of the function

e(x) = exp(2πix).

Therefore a typical exponential sum may take the form

Σ e(x_n)

summed over a finite sequence of real numbers

x_n.

If we allow some real coefficients a_n, to get the form

Σ a_ne(x_n),

it is the same as allowing exponents that are complex numbers. Both forms are certainly useful in applications. A large part of twentieth century analytic number theory was devoted to finding good estimates for these sums, a trend started by basic work of Hermann Weyl in diophantine approximation.

Estimates

The main thrust of the subject is that a sum

S = Σ e(x_n)

is trivially estimated by the number N of terms. That is, the absolute value

|S| ≤ N

by the triangle inequality, since each summand has absolute value 1. In applications one would like to do better. That involves proving some cancellation takes place, or in other words that this sum of complex numbers on the unit circle is not of numbers all with the same argument. The best that is it reasonable to hope for, is an estimate

|S| = O(√N)

which signifies, up to the implied constant in the big O notation, that the sum resembles a random walk in two dimensions.

Such an estimate can be considered ideal; it is unattainable in many of the major problems, and estimates

|S| = o(N)

have to be used, where the o(N) function represents only a small saving on the trivial estimate. A typical 'small saving' may be a factor of log N, for example. Even such a minor-seeming result in the right direction has to be referred all the way back to the structure of the initial sequence x_n, to show a degree of randomness. The techniques involved are ingenious and subtle.

History

Major advances in the subject were Van de Corput's method (c. 1920), related to the principle of stationary phase, and the later Vinogradov method(c.1930). The large sieve method (c.1960), the work of many researchers, is a relatively transparent general principle; but no one method has general application.

Types of exponential sum

Many types of sums are used in formulating particular problems; applications require usually a reduction to some known type, often by ingenious manipulations. Partial summation can be used to remove coefficients a_n, in many cases.

A basic distinction is between a complete exponential sum, which is typically a sum over all residue classes modulo some integer N (or more general finite ring), and an incomplete exponential sum where the range of summation is restricted by some inequality. Examples of complete exponential sums are Gauss sums and Kloosterman sums; these are in some sense finite field or finite ring analogues of the gamma function and some sort of Bessel function, respectively, and have many 'structural' properties. An example of an incomplete sum is the partial sum of the quadratic Gauss sum (indeed, the case investigated by Gauss). Here there are good estimates for sums over shorter ranges than the whole set of residue classes, because, in geometric terms, the partial sums approximate a Cornu's spiral; this implies massive cancellation.

Auxiliary types of sums occur in the theory, for example character sums; going back to Harold Davenport's thesis. The Weil conjectures had major applications to complete sums with domain restricted by polynomial conditions (i.e., along an algebraic variety over a finite field).

One of the most general types of exponential sum is the Weyl sum, with exponents 2πif(n) where f is a fairly general real-valued smooth function. These are the sums implicated in the distribution of the values f(n), according to Weyl's equidistribution criterion. There is a general theory of exponent pairs, which formulates estimates. An important case is where f is logarithmic, in relation with the Riemann zeta function.