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Sharp thresholds for Ramsey properties

Published online by Cambridge University Press:  27 February 2026

Ehud Friedgut
Affiliation:
Faculty of Mathematics and Computer Science, Weizmann Institute of Science , Rehovot, Israel; E-mail: ehud.friedgut@weizmann.ac.il
Eden Kuperwasser*
Affiliation:
School of Mathematical Sciences, Tel Aviv University , Tel Aviv, Israel
Wojciech Samotij
Affiliation:
School of Mathematical Sciences, Tel Aviv University , Tel Aviv, Israel; E-mail: samotij@tauex.tau.ac.il
Mathias Schacht
Affiliation:
Fachbereich Mathematik, Universität Hamburg , Hamburg, Germany; E-mail: schacht@math.uni-hamburg.de
*
E-mail: kuperwasser@mail.tau.ac.il (Corresponding author)

Abstract

In this work, we develop a unified framework for establishing sharp threshold results for various Ramsey properties. To achieve this, we view such properties as noncolourability of auxiliary hypergraphs. Our main technical result gives sufficient conditions on a sequence of such hypergraphs that guarantee that this noncolourability property has a sharp threshold in subhypergraphs induced by random subsets of the vertices.

Furthermore, we verify these conditions in several cases of interest. In the classical setting of Ramsey theory for graphs, we show that the property of being Ramsey for a graph H in r colours has a sharp threshold in $G_{n,p}$, for all $r \geqslant 2$ and all H in a class of graphs that includes all cliques and cycles. In the arithmetic setting, we establish sharpness of thresholds for the properties corresponding to van der Waerden’s theorem and Schur’s theorem, also in any number of colours.

Information

Type
Discrete Mathematics
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2026. Published by Cambridge University Press
Figure 0

Figure 1 Stars and constellations.

Figure 1

Figure 2 A Petersen star for $r=2$.