Convergence of Measures and Metrizability: Difference between revisions

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This article addresses narrow and wide convergence of probability measures.
This article addresses narrow and wide convergence of probability measures.
==Nets==
When speaking about general topological spaces that are not metric spaces, understanding the convergence of sequences does not determine topology or continuity. A generalization of sequences, known as <b>nets</b>, can be used to show continuity.<ref name="Kelley" /> Roughly, a net consists of a directed set <math>\{x_\gamma\}_{\gamma\in\Gamma}</math>: a function from a partially ordered set <math>\Gamma</math> such that for each <math>\gamma_1,\gamma_2\in\Gamma,\exists \gamma_3\in\Gamma</math> such that <math>\gamma_1,\gamma_2\preceq\gamma_3</math>. We say that this net converges to <math>x</math> if, for every open set <math>U\ni x</math>, there exists some large <math>a_U</math> such that for all <math>a_U\preceq a</math>, <math>x_{\gamma_a}\in U</math>.


==Weak-star Topologies==
==Weak-star Topologies==
Given a Banach space <math>X</math> and its Banach dual <math>X^*</math>, the dual can be endowed with the weakest topology that makes the evaluation maps at elements of <math>X</math> continuous. This is called the <b>weak-star topology relative to <math>X</math></b>. By Banach-Alaoglu, the unit ball of <math>X^*</math> (which we call <math>(X^*)_1</math>) with the weak-star topology is compact.
Given a Banach space <math>X</math> and its Banach dual <math>X^*</math>, the dual can be endowed with the weakest topology that makes the evaluation maps at elements of <math>X</math> continuous. This is called the [https://en.wikipedia.org/wiki/Weak_topology#Weak-*_topology weak-* topology on <math>X^*</math> relative to <math>X</math>]<ref name="KR" />. By [https://en.wikipedia.org/wiki/Banach%E2%80%93Alaoglu_theorem Banach-Alaoglu]<ref name="KR" />, the unit ball of <math>X^*</math> (which we call <math>(X^*)_1</math>) with the weak-star topology is compact.


In the case where <math>X</math> is norm separable, the weak-star topology on the unit ball of <math>X^*</math> can, in fact, be metrized. Fix a sequence <math>\{x_n\}_{n=1}^\infty</math> that is countable and dense in <math>X</math>. Define the metric <math>d</math> by <math> d(\phi,\psi):=\sum_{n=0}^\infty 2^{-n}\frac{|\phi(x_n)-\psi(x_n)|}{1+|\phi(x_n)-\psi(x_n)|}</math>. This is a sum of pseudometrics, necessarily convergent because each term is less than or equal to <math>2^{-n}</math>, and is nondegenerate because if <math>d(\phi,\psi)=0</math>, then <math> \phi(x_n)=\psi(x_n)</math> for each <math>x_n</math>, which would imply that the continuous functions <math>\phi,\psi</math> agreed on a dense subset of a metric space. The identity map from <math>((X^*)_1,w*)</math> to <math>((X^*)_1,d)</math> is continuous: choose a net <math>(\phi_\gamma)_{\gamma\in\Gamma} \to \phi</math>. Then for each <math>\epsilon>0</math>, perform the following truncation process: choose a large <math>N</math> so that <math>\sum_{n=N+1}^\infty 2^{-n}=2^{-N}<\frac{\epsilon}{2}</math>. Because <math>\phi_\gamma\xrightarrow{w*}\phi</math>, for each <math>n\in\{1,\ldots,N\}</math>, there is some large <math>\gamma_n</math> such that for all <math>\gamma\succeq\gamma_n</math>, <math>|\phi_\gamma(x_n)-\phi(x_n)|<\frac{\epsilon}{2\cdot N\cdot 2^{-n}}</math>. By the net order axioms, there is some large <math>\gamma_0\succeq\gamma_i\forall i\in\{1,\ldots,N\}</math>. So for each <math>\gamma\succeq \gamma_0</math>, <math>d(\phi_\gamma,\phi)<\sum_{n=1}^N \frac{1}{2N}+\sum_{n=N+1}^\infty 2^{-n}<\epsilon</math>. Now the identity map between the two spaces is a continuous bijection between a compact and a Hausdorff topological space, and is therefore a homeomorphism. So it metrizes the weak-star topology.
In the case where <math>X</math> is norm separable, the weak-star topology on the unit ball of <math>X^*</math> can, in fact, be metrized.<ref name="Rudin" /> Fix a sequence <math>\{x_n\}_{n=1}^\infty</math> that is countable and dense in <math>X</math>. Define the metric <math>d</math> by <math> d(\phi,\psi):=\sum_{n=0}^\infty 2^{-n}\frac{|\phi(x_n)-\psi(x_n)|}{1+|\phi(x_n)-\psi(x_n)|}</math>. This is a sum of pseudometrics, necessarily convergent because each term is less than or equal to <math>2^{-n}</math>, and is nondegenerate because if <math>d(\phi,\psi)=0</math>, then <math> \phi(x_n)=\psi(x_n)</math> for each <math>x_n</math>, which would imply that the continuous functions <math>\phi,\psi</math> agreed on a dense subset of a metric space. The identity map from <math>((X^*)_1,w*)</math> to <math>((X^*)_1,d)</math> is continuous: choose a convergent net in <math>(X^*)_1</math>, <math>(\phi_\gamma)_{\gamma\in\Gamma} \to \phi</math>. Then for each <math>\epsilon>0</math>, perform the following truncation process: choose a large <math>N</math> so that <math>\sum_{n=N+1}^\infty 2^{-n}=2^{-N}<\frac{\epsilon}{2}</math>. Because <math>\phi_\gamma\xrightarrow{w*}\phi</math>, for each <math>n\in\{1,\ldots,N\}</math>, there is some large <math>\gamma_n</math> such that for all <math>\gamma\succeq\gamma_n</math>, <math>|\phi_\gamma(x_n)-\phi(x_n)|<\frac{\epsilon}{2\cdot N\cdot 2^{-n}}</math>. By the net order axioms, there is some large <math>\gamma_0\succeq\gamma_i\forall i\in\{1,\ldots,N\}</math>. So for each <math>\gamma\succeq \gamma_0</math>, <math>d(\phi_\gamma,\phi)<\sum_{n=1}^N \frac{1}{2N}+\sum_{n=N+1}^\infty 2^{-n}<\epsilon</math>. Now the identity map between the two spaces is a continuous bijection between a compact and a Hausdorff topological space, and is therefore a homeomorphism. So it metrizes the weak-star topology.


==Metrizability for duals of <math>C(X)</math>-spaces==
==Metrizability for duals of <math>C(X)</math>-spaces==
If <math>X</math> is a compact Hausdorff metric space, <math>C(X)=C_b(X)=C_0(X)</math> is separable, due to the following argument: compact metric spaces are always separable. Pick a countable dense subset <math>\{x_n\}_{n\in\mathbb N}\subseteq X</math>, and consider the smallest <math>\mathbb Q</math>-algebra generated by the functions <math>d(x,x_n)</math>. This is a countable union of countable sets and therefore countable. As a subalgebra which separates points and contains the constant function, it must be dense by Stone-Weierstrass. So the unit ball of the dual of <math>C(X)</math> is metrizable.
If <math>X</math> is a compact Hausdorff metric space, <math>C(X)=C_b(X)=C_0(X)</math> is separable, due to the following argument: compact metric spaces are always separable<ref name="SE metric" />. Pick a countable dense subset <math>\{x_n\}_{n\in\mathbb N}\subseteq X</math>, and consider the smallest <math>\mathbb Q</math>-algebra generated by the functions <math>d(x,x_n)</math>. This is a countable union of countable sets and therefore countable. As a subalgebra which separates points and contains the constant function, it must be dense by Stone-Weierstrass. So the unit ball of the dual of <math>C(X)</math> is metrizable.


Conversely, assume that the unit ball of the dual of <math>C_b(X)</math> is metrizable. Then, because <math>X\rightarrow (C_b(X))^*</math> via point evaluation, which is a norm <math>1</math> map, and because the topology on <math>X</math> is exactly the topology of weak-star convergence in <math>C_b(X)^*</math>, this means that <math>X</math> is metrizable as well. So <math>X</math> is a metrizable space which lives inside a compact metrizable space. This is in fact equivalent to the Stone-Cech compactification of <math>X</math> being metrizable, which is quite rare.
Conversely, let <math>X</math> be a locally compact Hausdorff topological space, and assume that the unit ball of the dual of <math>C_b(X)</math> is metrizable. Then, because <math>X\rightarrow (C_b(X))^*</math> via point evaluation, which is a norm <math>1</math> map, and because the topology on <math>X</math> is exactly the topology of weak-star convergence in <math>C_b(X)^*</math>, this means that <math>X</math> is metrizable as well. So <math>X</math> is a metrizable space which lives inside a compact metrizable space. This is in fact equivalent to the Stone-Cech compactification of <math>X</math> being metrizable <ref name="SE stone cech" />, which is quite rare.


==Narrow Convergence==
==Narrow Convergence==
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==Wide Convergence==
==Wide Convergence==
Wide convergence is the weak-star convergence with respect to elements of <math>C_0(X)</math> rather than <math>C_b(X)</math>. As such, it is a weaker topology on the class of probability measures. When <math>X</math> is a locally compact separable metric space (in particular, locally compact metric spaces which are <math>\sigma</math>-compact are separable), we can find a separating family of functions which form a countable subalgebra. One way to do this is by taking, for each point <math>x_n</math> in a countable dense subset, a compact neighborhood <math>K_n\ni x_n</math> and taking a partition of unity subordinate to that compact, <math>\varphi_n</math>. Taking the <math>\mathbb Q</math>-algebra generated by this countable family of functions will separate points, which will make it dense in <math>C_0(X)</math> by Stone-Weierstrass. So <math>C_0(X)</math> is separable, which means that the unit ball of the dual is metrizable.
Wide convergence is the weak-star convergence with respect to elements of <math>C_0(X)</math> rather than <math>C_b(X)</math>. As such, it is a weaker topology on the class of probability measures. When <math>X</math> is a locally compact separable metric space (in particular, locally compact metric spaces which are <math>\sigma</math>-compact are separable), we can find a separating family of functions which form a countable subalgebra. One way to do this is by taking, for each point <math>x_n</math> in a countable dense subset, a compact neighborhood <math>K_n\ni x_n</math> and taking a partition of unity subordinate to that compact, <math>\varphi_n</math>. Taking the <math>\mathbb Q</math>-algebra generated by this countable family of functions will separate points, which will make it dense in <math>C_0(X)</math> by Stone-Weierstrass. So <math>C_0(X)</math> is separable, which means that the unit ball of the dual is metrizable.
==References==
<references>
<ref name="KR">Kadison, Ringrose. ''Fundamentals of the Theory of Operator Algebras, Volume I.'' Ch. 1.3, 1.6. Academic Press, 1983.</ref>
<ref name="Kelley">Kelley, ''General Topology'' Ch. 2. Springer, 1975.</ref>
<ref name="Rudin">Rudin, ''Functional Analysis'' Ch. 3. 1991.</ref>
<ref name="SE metric">[https://math.stackexchange.com/questions/974233/prove-if-x-is-a-compact-metric-space-then-x-is-separable/974252 Math StackExchange, ''Prove if <math>X</math> is a compact metric space, then <math>X</math> is separable.'' 2020.]</ref>
<ref name="SE stone cech">[https://math.stackexchange.com/questions/260794/stone-%c4%8cech-via-c-bx-cong-c-beta-x Math StackExchange, ''Stone-Cech via <math>C_b(X)\cong C(\beta X)</math>.'' 2020.]</ref>
</references>

Revision as of 22:07, 24 May 2020

This article addresses narrow and wide convergence of probability measures.

Nets

When speaking about general topological spaces that are not metric spaces, understanding the convergence of sequences does not determine topology or continuity. A generalization of sequences, known as nets, can be used to show continuity.[1] Roughly, a net consists of a directed set : a function from a partially ordered set such that for each such that . We say that this net converges to if, for every open set , there exists some large such that for all , .

Weak-star Topologies

Given a Banach space and its Banach dual , the dual can be endowed with the weakest topology that makes the evaluation maps at elements of continuous. This is called the weak-* topology on relative to [2]. By Banach-Alaoglu[2], the unit ball of (which we call ) with the weak-star topology is compact.

In the case where is norm separable, the weak-star topology on the unit ball of can, in fact, be metrized.[3] Fix a sequence that is countable and dense in . Define the metric by . This is a sum of pseudometrics, necessarily convergent because each term is less than or equal to , and is nondegenerate because if , then for each , which would imply that the continuous functions agreed on a dense subset of a metric space. The identity map from to is continuous: choose a convergent net in , . Then for each , perform the following truncation process: choose a large so that . Because , for each , there is some large such that for all , . By the net order axioms, there is some large . So for each , . Now the identity map between the two spaces is a continuous bijection between a compact and a Hausdorff topological space, and is therefore a homeomorphism. So it metrizes the weak-star topology.

Metrizability for duals of -spaces

If is a compact Hausdorff metric space, is separable, due to the following argument: compact metric spaces are always separable[4]. Pick a countable dense subset , and consider the smallest -algebra generated by the functions . This is a countable union of countable sets and therefore countable. As a subalgebra which separates points and contains the constant function, it must be dense by Stone-Weierstrass. So the unit ball of the dual of is metrizable.

Conversely, let be a locally compact Hausdorff topological space, and assume that the unit ball of the dual of is metrizable. Then, because via point evaluation, which is a norm map, and because the topology on is exactly the topology of weak-star convergence in , this means that is metrizable as well. So is a metrizable space which lives inside a compact metrizable space. This is in fact equivalent to the Stone-Cech compactification of being metrizable [5], which is quite rare.

Narrow Convergence

For every finite signed Radon measure on a locally compact Hausdorff space , there is some element such that . Moreover, letting denote the total variation of the measure, there is a net of functions such that , and . This means that , and can be isometrically identified with a subset of the dual. In particular, because the total variation norm does not increase with respect to continuous bounded functions, . Narrow convergence is weak-star convergence in with respect to : a net of measures converges to narrowly if, for every , .

Although in general the topology of narrow convergence is not metrizable on the unit ball -- for example, on any compact Hausdorff space which is not metrizable -- it is on the class of probability measures, so long as is separable. Take, again, a countable dense subset of , , and taking the family of functions . Let be the family of functions generated by taking infima of finitely many elements of , and let . This is still countable, and approximates integrals of elements of well weakly-star, so there is a metric on the probabilities by enumerating , and

Wide Convergence

Wide convergence is the weak-star convergence with respect to elements of rather than . As such, it is a weaker topology on the class of probability measures. When is a locally compact separable metric space (in particular, locally compact metric spaces which are -compact are separable), we can find a separating family of functions which form a countable subalgebra. One way to do this is by taking, for each point in a countable dense subset, a compact neighborhood and taking a partition of unity subordinate to that compact, . Taking the -algebra generated by this countable family of functions will separate points, which will make it dense in by Stone-Weierstrass. So is separable, which means that the unit ball of the dual is metrizable.

References

  1. Kelley, General Topology Ch. 2. Springer, 1975.
  2. 2.0 2.1 Kadison, Ringrose. Fundamentals of the Theory of Operator Algebras, Volume I. Ch. 1.3, 1.6. Academic Press, 1983.
  3. Rudin, Functional Analysis Ch. 3. 1991.
  4. Math StackExchange, Prove if is a compact metric space, then is separable. 2020.
  5. Math StackExchange, Stone-Cech via . 2020.