Every finite metric space has a large subset embeddable into R^d with small distortion

You need to know: Euclidean space {\mathbb R}^d, metric space (X,\rho) with metric \rho.

Background: We say that a subset S of metric space (X,\rho) can be embedded into metric space (Y,\rho') with distortion at most \alpha if there exists a function f:S\to Y such that m \rho(A,B) \leq \rho'(f(A),f(B)) \leq M \rho(A,B), \, \forall A,B \in S, where m,M>0 are constants such that \frac{M}{m}\leq \alpha.

The Theorem: On 4th December 2002, Yair Bartal, Nathan Linial, Manor Mendel, and Assaf Naor submitted to the Annals of Mathematics a paper in which they proved the existence of constant C>0 such that for every \alpha>1, every n-point metric space has a subset of size n^{1-C\frac{\log(2\alpha)}{\alpha}} which can be embedded into {\mathbb R}^d with distortion at most \alpha.

Short context: In 1985, Bourgain proved that every n-point metric space X can be embedded into {\mathbb R}^d with distortion at most C\log n (where the dimension d depends on n but the constant C does not). The bound C\log n is essentially sharp. The Theorem states, however, that reasonably large subsets of X can be embedded into {\mathbb R}^d with much smaller distortion. In a subsequent work Mendel and Naor showed that the Theorem holds for even larger subset of size n^{1-\frac{C}{\alpha}}, and that this is optimal up to the value of the constant C.

Links: Free arxiv version of the original paper is here, journal version is here. See also Section 5.8 of this book for an accessible description of the Theorem.

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