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Star refinement

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In mathematics, specifically in the study of topology and open covers of a topological space X, a star refinement is a particular kind of refinement of an open cover of X. The term has two similar but distinct usages. A related term sometimes used to differentiate the weaker of these two properties is the notion of a barycentric refinement.

Star refinements are used in the definition of a fully normal space, and in one among several equivalent formulations of a uniform space.

Definitions

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The general definition makes sense for arbitrary coverings and does not require a topology. Let X be a set and let 𝒰 be a covering of X, that is, X=⋃𝒰. Given a subset S of X, the star of S with respect to 𝒰 is the union of all the sets U∈𝒰 that intersect S, that is, st⁡(S,𝒰)=⋃{U∈𝒰:S∩U≠∅}.

Given a point x∈X, we write st⁡(x,𝒰) instead of st⁡({x},𝒰).

A covering 𝒰 of X is a refinement of a covering 𝒱 of X if every U∈𝒰 is contained in some V∈𝒱. The following are two special kinds of refinement. The covering 𝒰 is called a barycentric refinement of 𝒱 if for every x∈X the star st⁡(x,𝒰) is contained in some V∈𝒱.[1][2] The covering 𝒰 is called a star refinement of 𝒱 if for every U∈𝒰 the star st⁡(U,𝒰) is contained in some V∈𝒱.[3][2]

A space X is called fully normal if every open cover of X has a barycentric open refinement.

Properties and Examples

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Every star refinement of a cover is a barycentric refinement of that cover. The converse is not true, but a barycentric refinement of a barycentric refinement is a star refinement.[4][5][6][7]

Given a metric space X, let 𝒱={Bϵ(x):x∈X} be the collection of all open balls Bϵ(x) of a fixed radius ϵ>0. The collection 𝒰={Bϵ/2(x):x∈X} is a barycentric refinement of 𝒱, and the collection 𝒲={Bϵ/3(x):x∈X} is a star refinement of 𝒱.

By a theorem of A.H. Stone, for a T1 space being fully normal and being paracompact are equivalent. This was a landmark theorem and provided the first proof that metric spaces are paracompact. The proof is difficult, but simpler proofs of the paracompactness of metric spaces were later provided.

See also

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Notes

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  1. ↑ Dugundji 1966, Definition VIII.3.1, p. 167.
  2. 1 2 Willard 2004, Definition 20.1.
  3. ↑ Dugundji 1966, Definition VIII.3.3, p. 167.
  4. ↑ Dugundji 1966, Prop. VIII.3.4, p. 167.
  5. ↑ Willard 2004, Problem 20B.
  6. ↑ "Barycentric Refinement of a Barycentric Refinement is a Star Refinement". Mathematics Stack Exchange.
  7. ↑ Brandsma, Henno (2003). "On paracompactness, full normality and the like" (PDF).

References

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