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Diameters in supercritical random graphs via first passage percolation

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arxiv 0906.1840 v2 pith:5XTFB7CE submitted 2009-06-10 math.CO math.PR

classification math.COmath.PR
keywords epsilonsupercriticaldiameterphaseasymptoticemerginginftythroughout
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abstract

We study the diameter of $C_1$, the largest component of the Erd\H{o}s-R\'enyi random graph $G(n,p)$ in the emerging supercritical phase, i.e., for $p = \frac{1+\epsilon}n$ where $\epsilon^3 n \to \infty$ and $\epsilon=o(1)$. This parameter was extensively studied for fixed $\epsilon > 0$, yet results for $\epsilon=o(1)$ outside the critical window were only obtained very recently. Prior to this work, Riordan and Wormald gave precise estimates on the diameter, however these did not cover the entire supercritical regime (namely, when $\epsilon^3 n\to\infty$ arbitrarily slowly). {\L}uczak and Seierstad estimated its order throughout this regime, yet their upper and lower bounds differed by a factor of $1000/7$. We show that throughout the emerging supercritical phase, i.e. for any $\epsilon=o(1)$ with $\epsilon^3 n \to \infty$, the diameter of $C_1$ is with high probability asymptotic to $D(\epsilon,n)=(3/\epsilon)\log(\epsilon^3 n)$. This constitutes the first proof of the asymptotics of the diameter valid throughout this phase. The proof relies on a recent structure result for the supercritical giant component, which reduces the problem of estimating distances between its vertices to the study of passage times in first-passage percolation. The main advantage of our method is its flexibility. It also implies that in the emerging supercritical phase the diameter of the 2-core of $C_1$ is w.h.p. asymptotic to $(2/3)D(\epsilon,n)$, and the maximal distance in $C_1$ between any pair of kernel vertices is w.h.p. asymptotic to $(5/9)D(\epsilon,n)$.

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  1. Meeting and coalescence times for random walks in the largest component of the Erd\H{o}s-R\'enyi random graph

    math.PR 2026-07 accept novelty 8.0 of 10

    Expected meeting, coalescence, and voter-consensus times on the Erdős–Rényi giant are Θ(n) throughout the fixed-supercritical, slightly-supercritical, and critical regimes.

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