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, in the definition of a strongly paracompact space, and in one among several equivalent formulations of a uniform space.

Definitions

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 U𝒰 that intersect S, that is, st(S,𝒰)={U𝒰:SU}.

Given a point xX, 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 U𝒰 is contained in some V𝒱. The following are two special kinds of refinement. The covering 𝒰 is called a barycentric refinement of 𝒱 if for every xX the star st(x,𝒰) is contained in some V𝒱.[1][2] The covering 𝒰 is called a star refinement of 𝒱 if for every U𝒰 the star st(U,𝒰) is contained in some V𝒱.[3][2]

A space X is called strongly paracompact if every open cover of X has a star-finite open refinement. A space X is called fully normal if every open cover of X has a barycentric open refinement. By a theorem of A.H. Stone, for a T1 space being fully normal and being paracompact are equivalent. There are paracompact T1 spaces which are not strongly paracompact[4].

Properties and Examples

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.[5][6][7][8]

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

See also

Notes

References