Uniform integrability

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

Uniform integrability is an extension to the notion of a family of functions being dominated in L1 which is central in dominated convergence. Several textbooks on real analysis and measure theory use the following definition:

Definition A: Let (X,𝔐,μ) be a positive measure space. A set Φ⊂L1(μ) is called uniformly integrable if supf∈Φ‖f‖L1(μ)<∞, and to each ε>0 there corresponds a δ>0 such that

∫E|f|dμ<ε

whenever f∈Φ and μ(E)<δ.

Definition A is rather restrictive for infinite measure spaces. A more general definition of uniform integrability that works well in general measure spaces was introduced by G. A. Hunt.

Definition H: Let (X,𝔐,μ) be a positive measure space. A set Φ⊂L1(μ) is called uniformly integrable if and only if

infg∈L+1(μ)supf∈Φ∫{|f|>g}|f|dμ=0

where L+1(μ)={g∈L1(μ):g≥0}.


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 provides another equivalent notion to Hunt's. This equivalency is sometimes given as definition for uniform integrability.

Theorem 1: If (X,𝔐,μ) is a (positive) finite measure space, then a set Φ⊂L1(μ) is uniformly integrable if and only if

infg∈L+1(μ)supf∈Φ∫(|f|−g)+dμ=0

If in addition μ(X)<∞, then uniform integrability is equivalent to either of the following conditions

1. infa>0supf∈Φ∫(|f|−a)+dμ=0.

2. infa>0supf∈Φ∫{|f|>a}|f|dμ=0

When the underlying space (X,𝔐,μ) is σ-finite, Hunt's definition is equivalent to the following:

Theorem 2: Let (X,𝔐,μ) be a σ-finite measure space, and h∈L1(μ) be such that h>0 almost everywhere. A set Φ⊂L1(μ) is uniformly integrable if and only if supf∈Φ‖f‖L1(μ)<∞, and for any ε>0, there exists δ>0 such that

supf∈Φ∫A|f|dμ<ε

whenever ∫Ahdμ<δ.

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 h≡1 in Theorem 2.

Tightness, boundedness, equi-integrability and uniform integrability

Another concept associated with uniform integrability is that of tightness. In this article tightness is taken in a more general setting.

Definition: Suppose (X,𝔐,μ) is a measure space. Let 𝒦⊂𝔐 be a collection of sets of finite measure. A family Φ⊂L1(μ) is said to be tight with respect to 𝒦 if

infK∈𝒦supf∈Φ∫X∖K|f|dμ=0

When 𝒦=𝔐∩L1(μ), Φ is simply said to be tight.

When the measure space (X,𝔐,μ) is a metric space equipped with the Borel σ algebra, μ is a regular measure, and 𝒦 is the collection of all compact subsets of X, the notion of 𝒦-tightness discussed above coincides with the well known concept of tightness used in the analysis of regular measures in metric spaces

For σ-finite measure spaces, it can be shown that if a family Φ⊂L1(μ) is uniformly integrable, then Φ is tight. This is captured by the following result which is often used as definition of uniform integrability in the analysis literature:

Theorem 3: Suppose (X,𝔐,μ) is a σ-finite measure space. A family Φ⊂L1(μ) is uniformly integrable if and only if

  1. supf∈Φ‖f‖1<∞.
  2. infa>0supf∈Φ∫{|f|>a}|f|dμ=0
  3. Φ is tight.

When μ(X)<∞, condition 3 is redundant (see Theorem 1 above).

In many books in analysis , condition 2 in Theorem 3 is often replaced by another condition called equi-integrability:

Definition: A family 𝒞 of complex or real valued measurable functions is equi-integrable (or uniformly absolutely continuous with respect to a measure μ) if for any ε>0 there is δ>0 such that supf∈𝒞∫A|f|dμ<εwheneverμ(A)<δ

Theorem 3 then says that equi-integrability together with L1 boundedness and tightness (conditions (1) and (3) in Theorem 3) is equivalent to uniform integrability.

Relevant theorems

The following theorems describe very useful criteria for uniform integrability which have many applications in Analysis and Probability.

de la Vallée-Poussin theorem

Suppose (X,𝔐,μ) is a finite measure space. The family ℱ⊂L1(μ) is uniformly integrable if and only if there exists a function G:[0,∞)→[0,∞) such that limt→∞G(t)t=∞ and supf∈ℱ∫XG(|f|)dμ<∞. The function G can be chosen to be monotone increasing and convex.

Uniform integrability gives a characterization of weak compactness in L1.

Dunford–Pettis theorem

Suppose (X,𝔐,μ) is a σ-finite measure. A family ℱ⊂L1(μ) has compact closure in the weak topology σ(L1,L∞) if and only if ℱ is uniformly integrable.

Probability definition

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., that is,

1. A class 𝒞 of random variables is called uniformly integrable if:

or alternatively

2. A class 𝒞 of random variables is called uniformly integrable (UI) if for every ε>0 there exists K∈[0,∞) such that E⁡(|X|I|X|≥K)≤ε  for all X∈𝒞, where I|X|≥K is the indicator function I|X|≥K={1if |X|≥K,0if |X|<K..

The following results apply to the probabilistic definition.

Non-UI sequence of RVs. The area under the strip is always equal to 1, but Xn→0 pointwise.

Uniform integrability and stochastic ordering

A family of random variables {Xi}i∈I is uniformly integrable if and only if there exists a random variable X such that EX<∞ and |Xi|≤icxX for all i∈I, where ≤icx denotes the increasing convex stochastic order defined by A≤icxB if Eϕ(A)≤Eϕ(B) for all nondecreasing convex real functions ϕ.

Relation to convergence of random variables

A sequence {Xn} converges to X in the L1 norm if and only if it converges in measure to X 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. This is a generalization of Lebesgue's dominated convergence theorem, see Vitali convergence theorem.