A combinatorial approach to nonlinear spectral gaps
Dylan J. Altschuler, Pandelis Dodos, Konstantin Tikhomirov, Konstantinos Tyros

TL;DR
This paper introduces a combinatorial method to establish polynomial bounds on nonlinear spectral gaps for regular graphs in normed spaces with unconditional bases, advancing understanding of Poincaré inequalities and embeddings.
Contribution
It develops a new combinatorial framework based on long-range expansion to obtain optimal polynomial bounds on Poincaré constants for spaces with unconditional bases and finite cotype.
Findings
Polynomial dependence of Poincaré constants on cotype q
High probability of long-range expansion in random regular graphs
Lower bounds on cotype for low-distortion embeddings of random graphs
Abstract
A seminal open question of Pisier and Mendel--Naor asks whether every degree-regular graph which satisfies the classical discrete Poincar\'e inequality for scalar functions, also satisfies an analogous inequality for functions taking values in \textit{any} normed space with non-trivial cotype. Motivated by applications, it is also greatly important to quantify the dependence of the corresponding optimal Poincar\'e constant on the cotype . Works of Odell--Schlumprecht (1994), Ozawa (2004), and Naor (2014) make substantial progress on the former question by providing a positive answer for normed spaces which also have an unconditional basis, in addition to finite cotype. However, little is known in the way of quantitative estimates: the mentioned results imply a bound on the Poincar\'e constant depending super-exponentially on . We introduce a novel combinatorial framework for…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSemiconductor Lasers and Optical Devices · Advanced Fiber Optic Sensors
