Theorem 1.1 limit-shape conjecture for general rate vectors

Let rR\vec{\mathbf{r}}\in\mathscr{R} be a rate vector, let N1N\geq1, and suppose that N2TN^2T\to\infty. Theorem 1.1 concerns the spacetime limit shape of the KPZ equation in the upper-tail regime.

Theorem 1.1 limit-shape conjecture. The results of Theorem 1.1 hold for all rR\vec{\mathbf{r}}\in\mathscr{R} under N1N\geq1 and N2TN^2T\to\infty.

This extends the theorem beyond the parameter regime established in the paper. The surrounding discussion states that the limiting shape should still be described by the entropy solution of the backward equation with the corresponding terminal condition, while the behavior outside the concavity region is more complicated.

Sources & referencesView supporting material

Primary source

Yier Lin and Li-Cheng Tsai, “Spacetime limit shapes of the KPZ equation in the upper tails”, arXiv:2304.14380 (2023).

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