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Integral
The integral of a measurable function
on a measure space
is usually written
![]() |
(1) |
It is defined via the following steps:
- If
is the characteristic function
of a set
, then set

(2) - If
is a simple function (i.e. if
can be written as
for some finite collection
(3)
), then define

(4) - If
is a nonnegative measurable function (possibly attaining the value
at some points), then we define

(5) - For any measurable function
(possibly attaining the values
or
at some points), write
where
so that
and 
(6)
, and define the integral of
as
provided that
(7)
and
are not both
.
If
is Lebesgue measure
and
is any interval
in
then the integral is called the Lebesgue integral. If the Lebesgue integral of a function
on a set
exists and is finite (or, equivalently, if
), then
is said to be Lebesgue integrable. The Lebesgue integral equals the Riemann integral
everywhere the latter is defined; the advantage to the Lebesgue integral is that it is often well defined
even when the corresponding Riemann integral is undefined. For example, the Riemann integral of the characteristic function of the rationals
in
is undefined, while the Lebesgue integral of this function is simply the measure
of the rationals in
, which is 0. Moreover, the conditions under which Lebesgue integrals may be exchanged with each other or with limits
or derivatives, etc., are far less stringent, making the Lebesgue theory
a more convenient tool than the Riemann integral for theoretical purposes.
The introduction of the Lebesgue integral was a major advancement in real analysis, soon awakening a large interest in the scientific community. In 1916 Edward Burr Van Vleck, in "Bulletin of the American Mathematical Society", vol. 23, wrote: "This new integral of Lebesgue is proving itself a wonderful tool. I might compare it with a modern Krupp gun, so easily does it penetrate barriers which were impregnable."
