Before considering the generalization of the Riemann integral, it is necessary to define a simple function.
Assume that the function values are non-negative and the codomain of ϕ:R→R is a finite set {a1,a2,⋯,an}. If Ai=ϕ−1({ai})∈M satisfies, then ϕ is called a simple function. Simple functions have the following properties:
(i): If i=j, then Ai∩Aj=∅
(ii): k=1⨆nAk=R
(iii): ϕ(x)=k=1∑nak1Ak(x) is a measurable function.
Simple functions are inherently composed of three very manageable elements. Firstly, since the function values are non-negative, there is no need to consider the sign. Secondly, they are finite, allowing for free addition and subtraction. Thirdly, they are measurable. While the term simple is used in various ways across different fields of mathematics, in real analysis, it can certainly be considered the opposite of ‘complex.’ After defining such manageable and convenient simple functions, one can immediately think of a new integration that covers the Riemann integral.
Definition and Basic Properties
Lebesgue Integral of Simple Functions
When ϕ is a simple function and E∈M, the following is called the Lebesgue integral of the simple functionϕ.
∫Eϕdm:=k=1∑nakm(Ak∩E)
The Lebesgue integral of a simple function possesses the following properties:
[3]: If A,B∈M and A∩B=∅, then ∫A∪Bϕdm=∫Aϕdm+∫Bϕdm
Here, m denotes the Lebesgue measure. The condition of being a simple function is so strong and specific that it cannot be utilized in many places. By incorporating the idea of the partition method, a satisfactory ‘Lebesgue integral’ is formulated.
When ϕ is a simple function, and for the non-negative measurable functionf and E∈M, the following is termed the Lebesgue integral of the measurable functionf.
∫Efdm:=sup{∫Eϕdm0≤ϕ≤f}
The Lebesgue integral of a measurable function is characterized by these properties:
[1]’: For all r≥0, ∫Erfdm=r∫Efdm
[2]’: For two measurable functions f,g, if f≤g, then ∫Efdm≤∫Egdm
[3]’: If A,B∈M and A∩B=∅, then ∫A∪Bfdm=∫Afdm+∫Bfdm
[4]’: If A,B∈M and A⊂B, then ∫Afdm≤∫Bfdm
[5]’: If N∈N, then ∫Nfdm=0
[6]’: m(E)Einff≤∫Efdm≤m(E)Esupf
Besides these basic properties, the following widely utilized theorem is introduced.
For E:=f−1(0,∞), if m(E)=0, f is almost everywhere f=0. For proof, assume En:=f−1[n1,∞), then E=n=1⋃∞En and n→∞limEn=E hold true. Considering the simple function ϕn:=n11En≤f,
n1m(En)=∫Aϕndm≤∫Afdm=0
therefore
n1m(En)≤0
that is, for all n∈N, m(En)=0 holds.