# Dynamical universality classes of simple growth and lattice gas models

**Authors:** Jeffrey Kelling, G\'eza \'Odor, Sibylle Gemming

arXiv: 1701.03638 · 2017-12-19

## TL;DR

This study uses large-scale simulations of the 2D octahedron model to analyze surface growth universality classes, confirming theoretical conjectures and revealing finite size effects in KPZ and EW models.

## Contribution

It provides high-precision autocorrelation data, compares different stochastic dynamics, and supports the KPZ ansatz and Kallabis-Krug conjecture in 2+1 dimensions.

## Key findings

- Confirmed the KPZ growth exponent as 0.2414(2).
- Compared stochastic dynamics and their effects on correlations.
- Identified finite size corrections occurring before steady state.

## Abstract

Large scale, dynamical simulations have been performed for the two dimensional octahedron model, describing the Kardar-Parisi-Zhang (KPZ) for nonlinear, or the Edwards-Wilkinson (EW) class for linear surface growth. The autocorrelation functions of the heights and the dimer lattice gas variables are determined with high precision. Parallel random-sequential (RS) and two-sub-lattice stochastic dynamics (SCA) have been compared. The latter causes a constant correlation in the long time limit, but after subtracting it one can find the same height functions as in case of RS. On the other hand the ordered update alters the dynamics of the lattice gas variables, by increasing (decreasing) the memory effects for nonlinear (linear) models with respect to random-sequential. Additionally, we support the KPZ ansatz and the Kallabis-Krug conjecture in $2+1$ dimensions and provide a precise growth exponent value $\beta=0.2414(2)$. We show the emergence of finite size corrections, which occur long before the steady state roughness is reached.

## Full text

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## Figures

27 figures with captions in the complete paper: https://tomesphere.com/paper/1701.03638/full.md

## References

81 references — full list in the complete paper: https://tomesphere.com/paper/1701.03638/full.md

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Source: https://tomesphere.com/paper/1701.03638