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Uniform integrability
Mathematical concept From Wikipedia, the free encyclopedia
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In mathematics, uniform integrability is an important concept in real analysis, functional analysis and measure theory, and plays a vital role in the theory of martingales.
Measure-theoretic definition
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Uniform integrability is an extension to the notion of a family of functions being dominated in which is central in dominated convergence. Several textbooks on real analysis and measure theory use the following definition:[1]
Definition A: Let be a positive measure space. A set is called uniformly integrable if , and to each there corresponds a such that
whenever and
Definition A is rather restrictive for infinite measure spaces. A more general definition[2] of uniform integrability that works well in general measure spaces was introduced by G. A. Hunt.
Definition H: Let be a positive measure space. A set is called uniformly integrable if and only if
where .
Since Hunt's definition is equivalent to Definition A when the underlying measure space is finite (see Theorem 2 below), Definition H is widely adopted in Mathematics.
The following result[3] provides another equivalent notion to Hunt's. This equivalency is sometimes given as definition for uniform integrability.
Theorem 1: If is a (positive) finite measure space, then a set is uniformly integrable if and only if
If in addition , then uniform integrability is equivalent to either of the following conditions
1. .
2.
When the underlying space is -finite, Hunt's definition is equivalent to the following:
Theorem 2: Let be a -finite measure space, and be such that almost everywhere. A set is uniformly integrable if and only if , and for any , there exits such that
whenever .
A consequence of Theorems 1 and 2 is that equivalence of Definitions A and H for finite measures follows. Indeed, the statement in Definition A is obtained by taking in Theorem 2.
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Tightness and uniform integrability
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Another concept associated with uniform integrability is that of tightness. In this article tightness is taken in a more general setting.
Definition: Suppose measurable space is a measure space. Let be a collection of sets of finite measure. A family is tight with respect to if
A tight family with respect to is just said to be tight.
When the measure space is a metric space equipped with the Borel algebra, is a regular measure, and is the collection of all compact subsets of , the notion of -tightness discussed above coincides with the well known concept of tightness used in the analysis of regular measures in metric spaces
For -finite measure spaces, it can be shown that if a family is uniformly integrable, then is tight. This is capture by the following result which is often used as definition of uniform integrabiliy in the Analysis literature:
Theorem 3: Suppose is a finite measure space. A family is uniformly integrable if and only if
- .
- is tight.
When , condition 3 is redundant (see Theorem 1 above).
Condition 2 in Theorem 3 is sometimes replaced by what is called equi-integrability in many books in Analysis [4][5][6][7]: A family of complex or real valued measurable functions is equi-integrable (or uniformly absolutely continuous with respect to a measure ) if for any there is such that
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Relevant theorems
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The following theorem describes a very useful criterion for uniform integrability which is very useful in Probability theory.
de la Vallée-Poussin theorem[8][9]
Suppose is a finite measure space. The family is uniformly integrable if and only if there exists a function such that and The function can be chosen to be monotone increasing and convex.
Uniform integrability gives a characterization of weak compactness in .
Dunford–Pettis theorem[10][11]
Suppose is a -finite measure. A family has compact closure in the weak topology if and only if is uniformly integrable.
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Probability definition
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In probability theory, Definition A or the statement of Theorem 1 are often presented as definitions of uniform integrability using the notation expectation of random variables.,[12][13][14] that is,
1. A class of random variables is called uniformly integrable if:
- There exists a finite such that, for every in , and
- For every there exists such that, for every measurable such that and every in , .
or alternatively
2. A class of random variables is called uniformly integrable (UI) if for every there exists such that , where is the indicator function .
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Related corollaries
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The following results apply to the probabilistic definition.[15]
- Definition 1 could be rewritten by taking the limits as
- A non-UI sequence. Let , and define Clearly , and indeed for all n. However, and comparing with definition 1, it is seen that the sequence is not uniformly integrable.

- By using Definition 2 in the above example, it can be seen that the first clause is satisfied as norm of all s are 1 i.e., bounded. But the second clause does not hold as given any positive, there is an interval with measure less than and for all .
- If is a UI random variable, by splitting and bounding each of the two, it can be seen that a uniformly integrable random variable is always bounded in .
- If any sequence of random variables is dominated by an integrable, non-negative : that is, for all ω and n, then the class of random variables is uniformly integrable.
- A class of random variables bounded in () is uniformly integrable.
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Uniform integrability and stochastic ordering
A family of random variables is uniformly integrable if and only if[16] there exists a random variable such that and for all , where denotes the increasing convex stochastic order defined by if for all nondecreasing convex real functions .
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Relation to convergence of random variables
A sequence converges to in the norm if and only if it converges in measure to and it is uniformly integrable. In probability terms, a sequence of random variables converging in probability also converge in the mean if and only if they are uniformly integrable.[17] This is a generalization of Lebesgue's dominated convergence theorem, see Vitali convergence theorem.
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Citations
References
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