Obstructions to faster diameter computation: Asteroidal sets
Guillaume Ducoffe

TL;DR
This paper introduces new algorithms for efficiently computing the diameter and eccentricities in specific graph classes, overcoming obstructions posed by general computational hardness results.
Contribution
It provides the first deterministic algorithms with subquadratic runtime for diameter and eccentricity approximation in certain graph classes, improving upon previous complexity bounds.
Findings
Deterministic ${ m O}( ext{alpha}^3 m^{3/2})$-time diameter algorithm for graphs in $Ext_{\alpha}$
Linear-time diameter computation for graphs with bounded clique number
Approximate eccentricities within ${\rm O}( ext{alpha}^2 m)$ time
Abstract
An extremity is a vertex such that the removal of its closed neighbourhood does not increase the number of connected components. Let be the class of all connected graphs whose quotient graph obtained from modular decomposition contains no more than pairwise nonadjacent extremities. Our main contributions are as follows. First, we prove that the diameter of every -edge graph in can be computed in deterministic time. We then improve the runtime to linear for all graphs with bounded clique-number. Furthermore, we can compute an additive -approximation of all vertex eccentricities in deterministic time. This is in sharp contrast with general -edge graphs for which, under the Strong Exponential Time Hypothesis (SETH), one cannot compute the diameter in time for any…
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