Introduction
Let
be a measure space. From our study of integration[1], we know that if
are integrable functions, the following functions are also integrable:
, for
This shows that the set of integrable functions on any measurable space is a vector space. Furthermore, integration is a linear functional on this vector space, ie a linear function sending elements in our vector space to
, one would like to use integration to define a norm on our vector space. However, if one were to check the axioms for a norm, one finds integration fails to be a norm by taking
almost everywhere, then
. In other words, there are non zero functions which has a zero integral. This motivates our definition of
to be the set of integrable functions up to equivalence to sets of measure zero.
Space
In this section, we will construct
. These are sometimes called Lebesgue spaces.
Definition
Let
denote the set of integrable functions on
, ie
. Define an equivalence relation:
if
a.e. Then
. In some abuse of notation, we often refer to an element
as a function, even though it really denotes the equivalence class of all functions in
which are a.e. equivalent to
.
To see that
is indeed an equivalence relation, reflexivity and symmetry are immediate. Transitivity when
and
follows by considering the null set where
and
differ and similarly for
and
. Then see that the set where
and
differ is a subset of the union of the previous two null sets and hence is also a null set, so
.
To make sense of the definition, we need the following proposition:
Proposition: Let
, then the following are equivalent:
-
for all
-
a.e.
Since
a.e.,
a.e. Take a simple function,
, such that
, such
must be
a.e. Therefore,
Suppose the set
does not have measure zero. Then either
or
has nonzero measure, where
denotes
and
denotes
. WLOG, assume
has nonzero measure. Define the following sets
, then from continuity from below,
. This shows that there exists some
such that
, which implies that
, contradicting 1.
With the proposition, we define our norm on
to be
. This is indeed a norm since:
a.e
Completeness of
space
A space
with a metric
is said to be complete if for every Cauchy sequence
in
(that is,
as
) there exist
such that
in the sense that
as 
Riesz-Fischer Theorem
The vector space
is complete in its metric induced by the
-norm. [2]
Proof
See Stein and Shakarchi
Examples
References
- ↑ 1.0 1.1 Folland, Gerald B. (1999). Real Analysis: Modern Techniques and Their Applications, John Wiley and Sons, ISBN 0471317160, Second edition.
- ↑ Elias M. Stein and Rami Shakarchi(2005), Real Analysis: measure theory, integration, & hilbert spaces, first edition