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==<math>L^1(\mu)</math> Space==
==<math>L^1(\mu)</math> Space==
In this section, we will construct <math>L^1(\mu)</math>.  
In this section, we will construct <math>L^1(\mu)</math>. These are sometimes called Lebesgue spaces.


===Definition===
===Definition===
Let <math>L^1</math> denote the set of integrable functions on <math>X</math>, ie <math>\int |f| <\infty</math>. Define an equivalence relation: <math>f\sim g</math> if <math>f=g</math> a.e. Then <math>L^1(\mu)= L^1/\sim</math>.
Let <math>L^1</math> denote the set of integrable functions on <math>X</math>, ie <math>\int |f| <\infty</math>. Define an equivalence relation: <math>f\sim g</math> if <math>f=g</math> a.e. Then <math>L^1(\mu)= L^1/\sim</math>. In some abuse of notation, we often refer to an element <math>f \in L^1(\mu)</math> as a function, even though it really denotes the equivalence class of all functions in <math>L^1</math> which are a.e. equivalent to <math>f</math>.
 
To see that <math>\sim</math> is indeed an equivalence relation, reflexivity and symmetry are immediate. Transitivity when <math>f \sim g</math> and <math>g \sim h</math> follows by considering the null set where <math>f</math> and <math>g</math> differ and similarly for <math>g</math> and <math>h</math>. Then see that the set where <math>f</math> and <math>h</math> differ is a subset of the union of the previous two null sets and hence is also a null set, so <math>f \sim h</math>.


To make sense of the definition, we need the following proposition:
To make sense of the definition, we need the following proposition:
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==Completeness of <math>L^1 </math> space==
==Completeness of <math>L^1 </math> space==
A space <math>V</math> with a matirc <math>d</math> is said to be complete if for every Cauchy sequence <math>{x_k}</math> in <math>V</math> (that is, <math>d(x_l,x_k)\to 0</math> as <math>k,l \to \infty</math>) there exist <math>x \in V</math> such that <math>x_k \to x</math> in the sense that
A space <math>V</math> with a metric <math>d</math> is said to be complete if for every Cauchy sequence <math>{x_k}</math> in <math>V</math> (that is, <math>d(x_l,x_k)\to 0</math> as <math>k,l \to \infty</math>) there exist <math>x \in V</math> such that <math>x_k \to x</math> in the sense that
:<math>d(x_k,x)\to 0</math> as <math>k\to \infty</math>
:<math>d(x_k,x)\to 0</math> as <math>k\to \infty</math>
===Riesz-Fischer Theorem===
===Riesz-Fischer Theorem===
The vector space <math>L^1</math> is complete in its matric. <ref name="Stein">Elias M. Stein and Rami Shakarchi, Real Analysis: measure theory, integration, & hilbert spaces</ref>
The vector space <math>L^1</math> is complete in its metric induced by the <math>p</math>-norm. <ref name="Stein">Elias M. Stein and Rami Shakarchi(2005), Real Analysis: measure theory, integration, & hilbert spaces, first edition</ref>
====Proof====
====Proof====
See Stein and Shakarchi
See Stein and Shakarchi
==Examples==


==References==
==References==

Latest revision as of 10:50, 18 December 2020

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:

  1. , 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:

  1. for all
  2. a.e.

Proof[1]

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:

  1. 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. 1.0 1.1 Folland, Gerald B. (1999). Real Analysis: Modern Techniques and Their Applications, John Wiley and Sons, ISBN 0471317160, Second edition.
  2. Elias M. Stein and Rami Shakarchi(2005), Real Analysis: measure theory, integration, & hilbert spaces, first edition