Simple function

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In the

; as used in practice, they invariably are.

A basic example of a simple function is the

are simple.

Simple functions are used as a first stage in the development of theories of

Lebesgue integral

, because it is easy to define integration for a simple function and also it is straightforward to approximate more general functions by sequences of simple functions.

Definition

Formally, a simple function is a finite

. A simple function is a function ${\displaystyle f:X\to \mathbb {C} }$ of the form

${\displaystyle f(x)=\sum _{k=1}^{n}a_{k}{\mathbf {1} }_{A_{k}}(x),}$

where ${\displaystyle {\mathbf {1} }_{A}}$ is the indicator function of the set A.

Properties of simple functions

The sum, difference, and product of two simple functions are again simple functions, and multiplication by constant keeps a simple function simple; hence it follows that the collection of all simple functions on a given measurable space forms a commutative algebra over ${\displaystyle \mathbb {C} }$.

Integration of simple functions

If a

of f with respect to μ is

${\displaystyle \sum _{k=1}^{n}a_{k}\mu (A_{k}),}$

if all summands are finite.

Relation to Lebesgue integration

The above integral of simple functions can be extended to a more general class of functions, which is how the

is defined. This extension is based on the following fact.

Theorem. Any non-negative measurable function ${\displaystyle f\colon X\to \mathbb {R} ^{+}}$ is the pointwise limit of a monotonic increasing sequence of non-negative simple functions.

It is implied in the statement that the sigma-algebra in the co-domain ${\displaystyle \mathbb {R} ^{+}}$ is the restriction of the

${\displaystyle {\mathfrak {B}}(\mathbb {R} )}$ to ${\displaystyle \mathbb {R} ^{+}}$. The proof proceeds as follows. Let ${\displaystyle f}$ be a non-negative measurable function defined over the measure space ${\displaystyle (X,\Sigma ,\mu )}$. For each ${\displaystyle n\in \mathbb {N} }$, subdivide the co-domain of ${\displaystyle f}$ into ${\displaystyle 2^{2n}+1}$ intervals, ${\displaystyle 2^{2n}}$ of which have length ${\displaystyle 2^{-n}}$. That is, for each ${\displaystyle n}$, define

${\displaystyle I_{n,k}=\left[{\frac {k-1}{2^{n}}},{\frac {k}{2^{n}}}\right)}$ for ${\displaystyle k=1,2,\ldots ,2^{2n}}$, and ${\displaystyle I_{n,2^{2n}+1}=[2^{n},\infty )}$,

which are disjoint and cover the non-negative real line (${\displaystyle \mathbb {R} ^{+}\subseteq \cup _{k}I_{n,k},\forall n\in \mathbb {N} }$).

Now define the sets

${\displaystyle A_{n,k}=f^{-1}(I_{n,k})\,}$ for ${\displaystyle k=1,2,\ldots ,2^{2n}+1,}$

which are measurable (${\displaystyle A_{n,k}\in \Sigma }$) because ${\displaystyle f}$ is assumed to be measurable.

Then the increasing sequence of simple functions

${\displaystyle f_{n}=\sum _{k=1}^{2^{2n}+1}{\frac {k-1}{2^{n}}}{\mathbf {1} }_{A_{n,k}}}$

converges pointwise to ${\displaystyle f}$ as ${\displaystyle n\to \infty }$. Note that, when ${\displaystyle f}$ is bounded, the convergence is uniform.

See also

Bochner measurable function

References

• J. F. C. Kingman, S. J. Taylor. Introduction to Measure and Probability, 1966, Cambridge.
• S. Lang. Real and Functional Analysis, 1993, Springer-Verlag.
• W. Rudin. Real and Complex Analysis, 1987, McGraw-Hill.
• H. L. Royden. Real Analysis, 1968, Collier Macmillan.