In probability theory, there exist several different notions of convergence of sequences of random variables, including convergence in probability, convergence in distribution, and almost sure convergence. The different notions of convergence capture different properties about the sequence, with some notions of convergence being stronger than others. For example, convergence in distribution tells us about the limit distribution of a sequence of random variables. This is a weaker notion than convergence in probability, which tells us about the value a random variable will take, rather than just the distribution.
The concept is important in probability theory, and its applications to statistics and stochastic processes. The same concepts are known in more general mathematics as stochastic convergence and they formalize the idea that certain properties of a sequence of essentially random or unpredictable events can sometimes be expected to settle down into a behavior that is essentially unchanging when items far enough into the sequence are studied. The different possible notions of convergence relate to how such a behavior can be characterized: two readily understood behaviors are that the sequence eventually takes a constant value, and that values in the sequence continue to change but can be described by an unchanging probability distribution.
"Stochastic convergence" formalizes the idea that a sequence of essentially random or unpredictable events can sometimes be expected to settle into a pattern. The pattern may for instance be
Some less obvious, more theoretical patterns could be
These other types of patterns that may arise are reflected in the different types of stochastic convergence that have been studied.
While the above discussion has related to the convergence of a single series to a limiting value, the notion of the convergence of two series towards each other is also important, but this is easily handled by studying the sequence defined as either the difference or the ratio of the two series.
For example, if the average of n independent random variables Y i , i = 1 , … , n {\displaystyle Y_{i},\ i=1,\dots ,n} , all having the same finite mean and variance, is given by
then as n {\displaystyle n} tends to infinity, X n {\displaystyle X_{n}} converges in probability (see below) to the common mean, μ {\displaystyle \mu } , of the random variables Y i {\displaystyle Y_{i}} . This result is known as the weak law of large numbers. Other forms of convergence are important in other useful theorems, including the central limit theorem.
Throughout the following, we assume that ( X n ) {\displaystyle (X_{n})} is a sequence of random variables, and X {\displaystyle X} is a random variable, and all of them are defined on the same probability space ( Ω , F , P ) {\displaystyle (\Omega ,{\mathcal {F}},\mathbb {P} )} .
Loosely, with this mode of convergence, we increasingly expect to see the next outcome in a sequence of random experiments becoming better and better modeled by a given probability distribution. More precisely, the distribution of the associated random variable in the sequence becomes arbitrarily close to a specified fixed distribution.
Convergence in distribution is the weakest form of convergence typically discussed, since it is implied by all other types of convergence mentioned in this article. However, convergence in distribution is very frequently used in practice; most often it arises from application of the central limit theorem.
A sequence X 1 , X 2 , … {\displaystyle X_{1},X_{2},\ldots } of real-valued random variables, with cumulative distribution functions F 1 , F 2 , … {\displaystyle F_{1},F_{2},\ldots } , is said to converge in distribution, or converge weakly, or converge in law to a random variable X with cumulative distribution function F if
for every number x ∈ R {\displaystyle x\in \mathbb {R} } at which F {\displaystyle F} is continuous.
The requirement that only the continuity points of F {\displaystyle F} should be considered is essential. For example, if X n {\displaystyle X_{n}} are distributed uniformly on intervals ( 0 , 1 n ) {\displaystyle \left(0,{\frac {1}{n}}\right)} , then this sequence converges in distribution to the degenerate random variable X = 0 {\displaystyle X=0} . Indeed, F n ( x ) = 0 {\displaystyle F_{n}(x)=0} for all n {\displaystyle n} when x ≤ 0 {\displaystyle x\leq 0} , and F n ( x ) = 1 {\displaystyle F_{n}(x)=1} for all x ≥ 1 n {\displaystyle x\geq {\frac {1}{n}}} when n > 0 {\displaystyle n>0} . However, for this limiting random variable F ( 0 ) = 1 {\displaystyle F(0)=1} , even though F n ( 0 ) = 0 {\displaystyle F_{n}(0)=0} for all n {\displaystyle n} . Thus the convergence of cdfs fails at the point x = 0 {\displaystyle x=0} where F {\displaystyle F} is discontinuous.
Convergence in distribution may be denoted as
where L X {\displaystyle \scriptstyle {\mathcal {L}}_{X}} is the law (probability distribution) of X. For example, if X is standard normal we can write X n → d N ( 0 , 1 ) {\displaystyle X_{n}\,{\xrightarrow {d}}\,{\mathcal {N}}(0,\,1)} .
For random vectors { X 1 , X 2 , … } ⊂ R k {\displaystyle \left\{X_{1},X_{2},\dots \right\}\subset \mathbb {R} ^{k}} the convergence in distribution is defined similarly. We say that this sequence converges in distribution to a random k-vector X if
for every A ⊂ R k {\displaystyle A\subset \mathbb {R} ^{k}} which is a continuity set of X.
The definition of convergence in distribution may be extended from random vectors to more general random elements in arbitrary metric spaces, and even to the “random variables” which are not measurable — a situation which occurs for example in the study of empirical processes. This is the “weak convergence of laws without laws being defined” — except asymptotically.[1]
In this case the term weak convergence is preferable (see weak convergence of measures), and we say that a sequence of random elements {Xn} converges weakly to X (denoted as Xn ⇒ X) if
for all continuous bounded functions h.[2] Here E* denotes the outer expectation, that is the expectation of a “smallest measurable function g that dominates h(Xn)”.
The basic idea behind this type of convergence is that the probability of an “unusual” outcome becomes smaller and smaller as the sequence progresses.
The concept of convergence in probability is used very often in statistics. For example, an estimator is called consistent if it converges in probability to the quantity being estimated. Convergence in probability is also the type of convergence established by the weak law of large numbers.
A sequence {Xn} of random variables converges in probability towards the random variable X if for all ε > 0
More explicitly, let Pn(ε) be the probability that Xn is outside the ball of radius ε centered at X. Then Xn is said to converge in probability to X if for any ε > 0 and any δ > 0 there exists a number N (which may depend on ε and δ) such that for all n ≥ N, Pn(ε) < δ (the definition of limit).
Notice that for the condition to be satisfied, it is not possible that for each n the random variables X and Xn are independent (and thus convergence in probability is a condition on the joint cdf's, as opposed to convergence in distribution, which is a condition on the individual cdf's), unless X is deterministic like for the weak law of large numbers. At the same time, the case of a deterministic X cannot, whenever the deterministic value is a discontinuity point (not isolated), be handled by convergence in distribution, where discontinuity points have to be explicitly excluded.
Convergence in probability is denoted by adding the letter p over an arrow indicating convergence, or using the "plim" probability limit operator:
For random elements {Xn} on a separable metric space (S, d), convergence in probability is defined similarly by[6]
Not every sequence of random variables which converges to another random variable in distribution also converges in probability to that random variable. As an example, consider a sequence of standard normal random variables X n {\displaystyle X_{n}} and a second sequence Y n = ( − 1 ) n X n {\displaystyle Y_{n}=(-1)^{n}X_{n}} . Notice that the distribution of Y n {\displaystyle Y_{n}} is equal to the distribution of X n {\displaystyle X_{n}} for all n {\displaystyle n} , but: P ( | X n − Y n | ≥ ϵ ) = P ( | X n | ⋅ | ( 1 − ( − 1 ) n ) | ≥ ϵ ) {\displaystyle P(|X_{n}-Y_{n}|\geq \epsilon )=P(|X_{n}|\cdot |(1-(-1)^{n})|\geq \epsilon )}
which does not converge to 0 {\displaystyle 0} . So we do not have convergence in probability.
This is the type of stochastic convergence that is most similar to pointwise convergence known from elementary real analysis.
To say that the sequence Xn converges almost surely or almost everywhere or with probability 1 or strongly towards X means that P ( lim n → ∞ X n = X ) = 1. {\displaystyle \mathbb {P} \!\left(\lim _{n\to \infty }\!X_{n}=X\right)=1.}
This means that the values of Xn approach the value of X, in the sense that events for which Xn does not converge to X have probability 0 (see Almost surely). Using the probability space ( Ω , F , P ) {\displaystyle (\Omega ,{\mathcal {F}},\mathbb {P} )} and the concept of the random variable as a function from Ω to R, this is equivalent to the statement P ( ω ∈ Ω : lim n → ∞ X n ( ω ) = X ( ω ) ) = 1. {\displaystyle \mathbb {P} {\Bigl (}\omega \in \Omega :\lim _{n\to \infty }X_{n}(\omega )=X(\omega ){\Bigr )}=1.}
Using the notion of the limit superior of a sequence of sets, almost sure convergence can also be defined as follows: P ( lim sup n → ∞ { ω ∈ Ω : | X n ( ω ) − X ( ω ) | > ε } ) = 0 for all ε > 0. {\displaystyle \mathbb {P} {\Bigl (}\limsup _{n\to \infty }{\bigl \{}\omega \in \Omega :|X_{n}(\omega )-X(\omega )|>\varepsilon {\bigr \}}{\Bigr )}=0\quad {\text{for all}}\quad \varepsilon >0.}
Almost sure convergence is often denoted by adding the letters a.s. over an arrow indicating convergence:
For generic random elements {Xn} on a metric space ( S , d ) {\displaystyle (S,d)} , convergence almost surely is defined similarly: P ( ω ∈ Ω : d ( X n ( ω ) , X ( ω ) ) ⟶ n → ∞ 0 ) = 1 {\displaystyle \mathbb {P} {\Bigl (}\omega \in \Omega \colon \,d{\big (}X_{n}(\omega ),X(\omega ){\big )}\,{\underset {n\to \infty }{\longrightarrow }}\,0{\Bigr )}=1}
Consider a sequence { X n } {\displaystyle \{X_{n}\}} of independent random variables such that P ( X n = 1 ) = 1 n {\displaystyle P(X_{n}=1)={\frac {1}{n}}} and P ( X n = 0 ) = 1 − 1 n {\displaystyle P(X_{n}=0)=1-{\frac {1}{n}}} . For 0 < ε < 1 / 2 {\displaystyle 0<\varepsilon <1/2} we have P ( | X n | ≥ ε ) = 1 n {\displaystyle P(|X_{n}|\geq \varepsilon )={\frac {1}{n}}} which converges to 0 {\displaystyle 0} hence X n → 0 {\displaystyle X_{n}\to 0} in probability.
Since ∑ n ≥ 1 P ( X n = 1 ) → ∞ {\displaystyle \sum _{n\geq 1}P(X_{n}=1)\to \infty } and the events { X n = 1 } {\displaystyle \{X_{n}=1\}} are independent, second Borel Cantelli Lemma ensures that P ( lim sup n { X n = 1 } ) = 1 {\displaystyle P(\limsup _{n}\{X_{n}=1\})=1} hence the sequence { X n } {\displaystyle \{X_{n}\}} does not converge to 0 {\displaystyle 0} almost everywhere (in fact the set on which this sequence does not converge to 0 {\displaystyle 0} has probability 1 {\displaystyle 1} ).
To say that the sequence of random variables (Xn) defined over the same probability space (i.e., a random process) converges surely or everywhere or pointwise towards X means
∀ ω ∈ Ω : lim n → ∞ X n ( ω ) = X ( ω ) , {\displaystyle \forall \omega \in \Omega \colon \ \lim _{n\to \infty }X_{n}(\omega )=X(\omega ),}
where Ω is the sample space of the underlying probability space over which the random variables are defined.
This is the notion of pointwise convergence of a sequence of functions extended to a sequence of random variables. (Note that random variables themselves are functions).
{ ω ∈ Ω : lim n → ∞ X n ( ω ) = X ( ω ) } = Ω . {\displaystyle \left\{\omega \in \Omega :\lim _{n\to \infty }X_{n}(\omega )=X(\omega )\right\}=\Omega .}
Sure convergence of a random variable implies all the other kinds of convergence stated above, but there is no payoff in probability theory by using sure convergence compared to using almost sure convergence. The difference between the two only exists on sets with probability zero. This is why the concept of sure convergence of random variables is very rarely used.
Given a real number r ≥ 1, we say that the sequence Xn converges in the r-th mean (or in the Lr-norm) towards the random variable X, if the r-th absolute moments E {\displaystyle \mathbb {E} } (|Xn|r ) and E {\displaystyle \mathbb {E} } (|X|r ) of Xn and X exist, and
where the operator E denotes the expected value. Convergence in r-th mean tells us that the expectation of the r-th power of the difference between X n {\displaystyle X_{n}} and X {\displaystyle X} converges to zero.
This type of convergence is often denoted by adding the letter Lr over an arrow indicating convergence:
The most important cases of convergence in r-th mean are:
Convergence in the r-th mean, for r ≥ 1, implies convergence in probability (by Markov's inequality). Furthermore, if r > s ≥ 1, convergence in r-th mean implies convergence in s-th mean. Hence, convergence in mean square implies convergence in mean.
Additionally,
The converse is not necessarily true, however it is true if X n → p X {\displaystyle {\overset {}{X_{n}\,\xrightarrow {p} \,X}}} (by a more general version of Scheffé's lemma).
Provided the probability space is complete:
The chain of implications between the various notions of convergence are noted in their respective sections. They are, using the arrow notation:
These properties, together with a number of other special cases, are summarized in the following list:
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This article incorporates material from the Citizendium article "Stochastic convergence", which is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License but not under the GFDL.