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Tightness of measures

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In mathematics, tightness is a concept in measure theory. The intuitive idea is that a given collection of measures does not "escape to infinity".

Definitions

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Let ( X , T ) {\displaystyle (X,T)} {\displaystyle (X,T)} be a Hausdorff space, and let Σ {\displaystyle \Sigma } {\displaystyle \Sigma } be a σ-algebra on X {\displaystyle X} {\displaystyle X} that contains the topology T {\displaystyle T} {\displaystyle T}. (Thus, every open subset of X {\displaystyle X} {\displaystyle X} is a measurable set and Σ {\displaystyle \Sigma } {\displaystyle \Sigma } is at least as fine as the Borel σ-algebra on X {\displaystyle X} {\displaystyle X}.) Let M {\displaystyle M} {\displaystyle M} be a collection of (possibly signed or complex) measures defined on Σ {\displaystyle \Sigma } {\displaystyle \Sigma }. The collection M {\displaystyle M} {\displaystyle M} is called tight (or sometimes uniformly tight) if, for any ε > 0 {\displaystyle \varepsilon >0} {\displaystyle \varepsilon >0}, there is a compact subset K ε {\displaystyle K_{\varepsilon }} {\displaystyle K_{\varepsilon }} of X {\displaystyle X} {\displaystyle X} such that, for all measures μ M {\displaystyle \mu \in M} {\displaystyle \mu \in M},

| μ | ( X K ε ) < ε . {\displaystyle |\mu |(X\setminus K_{\varepsilon })<\varepsilon .} {\displaystyle |\mu |(X\setminus K_{\varepsilon })<\varepsilon .}

where | μ | {\displaystyle |\mu |} {\displaystyle |\mu |} is the total variation measure of μ {\displaystyle \mu } {\displaystyle \mu }. Very often, the measures in question are probability measures, so the last part can be written as

μ ( K ε ) > 1 ε . {\displaystyle \mu (K_{\varepsilon })>1-\varepsilon .,円} {\displaystyle \mu (K_{\varepsilon })>1-\varepsilon .,円}

If a tight collection M {\displaystyle M} {\displaystyle M} consists of a single measure μ {\displaystyle \mu } {\displaystyle \mu }, then (depending upon the author) μ {\displaystyle \mu } {\displaystyle \mu } may either be said to be a tight measure or to be an inner regular measure .

If Y {\displaystyle Y} {\displaystyle Y} is an X {\displaystyle X} {\displaystyle X}-valued random variable whose probability distribution on X {\displaystyle X} {\displaystyle X} is a tight measure then Y {\displaystyle Y} {\displaystyle Y} is said to be a separable random variable or a Radon random variable.

Another equivalent criterion of the tightness of a collection M {\displaystyle M} {\displaystyle M} is sequential weak compactness. We say the family M {\displaystyle M} {\displaystyle M} of probability measures is sequentially weakly compact if for every sequence { μ n } {\displaystyle \left\{\mu _{n}\right\}} {\displaystyle \left\{\mu _{n}\right\}} from the family, there is a subsequence of measures that converges weakly to some probability measure μ {\displaystyle \mu } {\displaystyle \mu }. It can be shown that a family of measures is tight if and only if it is sequentially weakly compact.

Examples

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Compact spaces

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If X {\displaystyle X} {\displaystyle X} is a metrizable compact space, then every collection of (possibly complex) measures on X {\displaystyle X} {\displaystyle X} is tight. This is not necessarily so for non-metrisable compact spaces. If we take [ 0 , ω 1 ] {\displaystyle [0,\omega _{1}]} {\displaystyle [0,\omega _{1}]} with its order topology, then there exists a measure μ {\displaystyle \mu } {\displaystyle \mu } on it that is not inner regular. Therefore, the singleton { μ } {\displaystyle \{\mu \}} {\displaystyle \{\mu \}} is not tight.

Polish spaces

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If X {\displaystyle X} {\displaystyle X} is a Polish space, then every finite measure on X {\displaystyle X} {\displaystyle X} is tight; this is Ulam's theorem. Furthermore, by Prokhorov's theorem, a collection of probability measures on X {\displaystyle X} {\displaystyle X} is tight if and only if it is precompact in the topology of weak convergence.

A collection of point masses

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Consider the real line R {\displaystyle \mathbb {R} } {\displaystyle \mathbb {R} } with its usual Borel topology. Let δ x {\displaystyle \delta _{x}} {\displaystyle \delta _{x}} denote the Dirac measure, a unit mass at the point x {\displaystyle x} {\displaystyle x} in R {\displaystyle \mathbb {R} } {\displaystyle \mathbb {R} }. The collection M 1 := { δ n n N } {\displaystyle M_{1}:=\{\delta _{n}\mid n\in \mathbb {N} \}} {\displaystyle M_{1}:=\{\delta _{n}\mid n\in \mathbb {N} \}} is not tight, since the compact subsets of R {\displaystyle \mathbb {R} } {\displaystyle \mathbb {R} } are precisely the closed and bounded subsets, and any such set, since it is bounded, has δ n {\displaystyle \delta _{n}} {\displaystyle \delta _{n}}-measure zero for large enough n {\displaystyle n} {\displaystyle n}. On the other hand, the collection M 2 := { δ 1 / n n N } {\displaystyle M_{2}:=\{\delta _{1/n}\mid n\in \mathbb {N} \}} {\displaystyle M_{2}:=\{\delta _{1/n}\mid n\in \mathbb {N} \}} is tight: the compact interval [ 0 , 1 ] {\displaystyle [0,1]} {\displaystyle [0,1]} will work as K ε {\displaystyle K_{\varepsilon }} {\displaystyle K_{\varepsilon }} for any ε > 0 {\displaystyle \varepsilon >0} {\displaystyle \varepsilon >0}. In general, a collection of Dirac delta measures on R n {\displaystyle \mathbb {R} ^{n}} {\displaystyle \mathbb {R} ^{n}} is tight if, and only if, the collection of their supports is bounded.

A collection of Gaussian measures

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Consider n {\displaystyle n} {\displaystyle n}-dimensional Euclidean space R n {\displaystyle \mathbb {R} ^{n}} {\displaystyle \mathbb {R} ^{n}} with its usual Borel topology and σ-algebra. Consider a collection of Gaussian measures Γ = { γ i i I } , {\displaystyle \Gamma =\{\gamma _{i}\mid i\in I\},} {\displaystyle \Gamma =\{\gamma _{i}\mid i\in I\},} where the measure γ i {\displaystyle \gamma _{i}} {\displaystyle \gamma _{i}} has expected value (mean) m i R n {\displaystyle m_{i}\in \mathbb {R} ^{n}} {\displaystyle m_{i}\in \mathbb {R} ^{n}} and covariance matrix C i R n × n {\displaystyle C_{i}\in \mathbb {R} ^{n\times n}} {\displaystyle C_{i}\in \mathbb {R} ^{n\times n}}. Then the collection Γ {\displaystyle \Gamma } {\displaystyle \Gamma } is tight if, and only if, the collections { m i i I } R n {\displaystyle \{m_{i}\mid i\in I\}\subseteq \mathbb {R} ^{n}} {\displaystyle \{m_{i}\mid i\in I\}\subseteq \mathbb {R} ^{n}} and { C i i I } R n × n {\displaystyle \{C_{i}\mid i\in I\}\subseteq \mathbb {R} ^{n\times n}} {\displaystyle \{C_{i}\mid i\in I\}\subseteq \mathbb {R} ^{n\times n}} are both bounded.

Tightness and convergence

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Tightness is often a necessary criterion for proving the weak convergence of a sequence of probability measures, especially when the measure space has infinite dimension. See

Tightness and stochastic ordering

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A family of real-valued random variables { X i } i I {\displaystyle \{X_{i}\}_{i\in I}} {\displaystyle \{X_{i}\}_{i\in I}} is tight if and only if there exists an almost surely finite random variable X {\displaystyle X} {\displaystyle X} such that | X i | s t X {\displaystyle |X_{i}|\leq _{\mathrm {st} }X} {\displaystyle |X_{i}|\leq _{\mathrm {st} }X} for all i I {\displaystyle i\in I} {\displaystyle i\in I}, where s t {\displaystyle \leq _{\mathrm {st} }} {\displaystyle \leq _{\mathrm {st} }} denotes the stochastic order defined by A s t B {\displaystyle A\leq _{\mathrm {st} }B} {\displaystyle A\leq _{\mathrm {st} }B} if E [ ϕ ( A ) ] E [ ϕ ( B ) ] {\displaystyle \mathbb {E} [\phi (A)]\leq \mathbb {E} [\phi (B)]} {\displaystyle \mathbb {E} [\phi (A)]\leq \mathbb {E} [\phi (B)]} for all nondecreasing functions ϕ {\displaystyle \phi } {\displaystyle \phi }. [1]

Exponential tightness

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A strengthening of tightness is the concept of exponential tightness, which has applications in large deviations theory. A family of probability measures ( μ δ ) δ > 0 {\displaystyle (\mu _{\delta })_{\delta >0}} {\displaystyle (\mu _{\delta })_{\delta >0}} on a Hausdorff topological space X {\displaystyle X} {\displaystyle X} is said to be exponentially tight if, for any ε > 0 {\displaystyle \varepsilon >0} {\displaystyle \varepsilon >0}, there is a compact subset K ε {\displaystyle K_{\varepsilon }} {\displaystyle K_{\varepsilon }} of X {\displaystyle X} {\displaystyle X} such that

lim sup δ 0 δ log μ δ ( X K ε ) < ε . {\displaystyle \limsup _{\delta \downarrow 0}\delta \log \mu _{\delta }(X\setminus K_{\varepsilon })<-\varepsilon .} {\displaystyle \limsup _{\delta \downarrow 0}\delta \log \mu _{\delta }(X\setminus K_{\varepsilon })<-\varepsilon .}

References

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  1. ^ Leskelä, L.; Vihola, M. (2013). "Stochastic order characterization of uniform integrability and tightness". Statistics and Probability Letters. 83 (1): 382–389. arXiv:1106.0607 . doi:10.1016/j.spl.2012年09月02日3.
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