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a generalization of the classical concept of the integral for the case of unbounded functions or functions defined on an infinite interval of integration. The definite integral as the limit of Riemann sums can exist (can have a definite finite value) only for bounded functions defined on a finite interval. Therefore, if the interval of integration or the integrand is not bounded, then still another limiting process is required in order to define the integral. Integrals thus obtained are called improper integrals.
If a function f (x) is integrable on any finite interval [a, N] and if
exists, then the latter is said to be the improper integral of f(x) on the interval [a, ∞] and is denoted by
In this case, the improper integral is said to converge. When this limit and thus also the improper integral do not exist, then the improper integral is said to diverge. For example, dx converges for γ > 1 and diverges for γ ≤ 1. Improper integrals are similarly defined on the intervals [-∞ ,b] and [—∞ ,∞].
If a function f(x), defined on an interval [a, b], is not bounded in a neighborhood of the point a but is integrable on any interval [a + ∊, b], 0 < e < b − a, and if
exists, then this limit is called the improper integral of f(x) on [a, b] and is usually written as an ordinary integral
We proceed in a similar manner if f(x) is not bounded in a neighborhood of the point b.
If the improper integral exists, then it is said that the improper integral is absolutely convergent; if the latter integrals, however, converge while the former diverge, then the improper integral is said to be conditionally convergent.
Problems leading to improper integrals were examined in geometrical form by E. Torricelli and P. de Fermat in 1644. Precise definitions of improper integrals were given by A. Cauchy in 1823. The distinction between conditionally and absolutely convergent integrals was made by G. Stokes and P. G. L. Dirichlet (1854). A number of mathematical works in the 19th century were devoted to the evaluation of improper integrals in cases where the corresponding antiderivatives could not be expressed in terms of elementary functions. The basic methods of evaluating improper integrals are differentiation, integration with respect to a parameter, series expansion, and application of the theory of residues. The values of many improper integrals are given in various tables.
Improper integrals are very important in many areas of mathematical analysis and in applications. In the theory of special functions (cylindrical functions, orthogonal polynomials), one of the fundamental research methods is the representation of the functions in the form of improper integrals depending on a parameter. A relevant example is the gamma function, ┌ (ɑ) = . Improper integrals include the Fourier integral, as well as the integrals encountered in other integral transforms. Solutions of boundary-value problems in mathematical physics are written as multiple improper integrals with an unbounded function as integrand. The improper integral
is very important in probability theory, as is the improper integral
in the theory of the diffraction of light.
In a number of cases, a definite value may be assigned to a divergent improper integral. In particular, if the integral f(x) dx diverges but the symmetric limit
exists, then A is called the Cauchy principal value of f(x) dx. Thus, the Cauchy principal value of
is 0. The Cauchy principal value of an improper integral of an unbounded function is similarly defined. A theory of integral equations involving improper integrals understood in the Cauchy principal value sense has been constructed by N. I. Muskhelishvili and his students.
REFERENCESSmirnov, V. I. Kurs vysshei matematiki, 20th ed., vol. 2. Moscow-Leningrad, 1967.
Fikhtengol’ts, G. M. Kurs differentsial’nogo i integral’nogo ischisleniia, 7th ed., vol. 2. Moscow, 1969.
Kudriavtsev, L. D. Matematicheskii analiz, vol. 1. Moscow, 1970.