The AKPZ universality-class conjecture for two-dimensional growth models

Let v()v(\cdot) be the speed function of a reasonable (2+1)(2+1)-dimensional growth model, and let HρH_\rho be the Hessian of v()v(\cdot) computed at the slope ρ\rho. Write α\alpha for the spatial growth exponent and β\beta for the temporal growth exponent. AKPZ universality conjecture. If det(Hρ)>0\det(H_\rho)>0, then height fluctuations grow in time as tβt^\beta for some model-independent β>0\beta>0, and height fluctuations in stationary states grow as distance to the power 2β/(β+1)2\beta/(\beta+1). If instead det(Hρ)0\det(H_\rho)\leq 0, then β=α=0\beta=\alpha=0 and stationary states have the same spatial height correlations as a massless Gaussian field. This conjecture predicts a distinction between the isotropic KPZ and anisotropic KPZ universality classes: the former has nonzero growth exponents, while the latter has logarithmic fluctuations and Gaussian-field spatial correlations. The assertion remains unproved for the relevant (2+1)(2+1)-dimensional growth models.

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Primary source

F. L. Toninelli, “(2+1)-dimensional interface dynamics: mixing time, hydrodynamic limit and Anisotropic KPZ growth”, arXiv:1711.05571 (2017).

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