# Tightness and tails of the maximum in 3D Ising interfaces

**Authors:** Reza Gheissari, Eyal Lubetzky

arXiv: 1907.07173 · 2020-05-14

## TL;DR

This paper investigates the maximum height of the interface in the 3D Ising model at low temperatures, showing tightness and Gumbel tail behavior of the centered maxima, with detailed large deviation analysis of surface pillars.

## Contribution

It establishes the uniform tightness and Gumbel tail bounds for the maximum interface height, advancing understanding of surface fluctuations in the 3D Ising model.

## Key findings

- Centered maxima are uniformly tight.
- Maxima exhibit Gumbel tail behavior.
- Detailed large deviation shape of high-reaching pillars.

## Abstract

Consider the 3D Ising model on a box of side length $n$ with minus boundary conditions above the $xy$-plane and plus boundary conditions below it. At low temperatures, Dobrushin (1972) showed that the interface separating the predominantly plus and predominantly minus regions is localized: its height above a fixed point has exponential tails. Recently, the authors proved a law of large numbers for the maximum height $M_n$ of this interface: for every $\beta$ large, $M_n/ \log n\to c_\beta$ in probability as $n\to\infty$.   Here we show that the laws of the centered maxima $(M_n - \mathbb{E}[M_n])_{n\geq 1}$ are uniformly tight. Moreover, even though this sequence does not converge, we prove that it has uniform upper and lower Gumbel tails (exponential right tails and doubly exponential left tails). Key to the proof is a sharp (up to $O(1)$ precision) understanding of the surface large deviations. This includes, in particular, the shape of a pillar that reaches near-maximum height, even at its base, where the interactions with neighboring pillars are dominant.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1907.07173/full.md

## References

25 references — full list in the complete paper: https://tomesphere.com/paper/1907.07173/full.md

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Source: https://tomesphere.com/paper/1907.07173