# Exact short-time height distribution in 1D KPZ equation with Brownian   initial condition

**Authors:** Alexandre Krajenbrink, Pierre Le Doussal

arXiv: 1705.04654 · 2017-08-23

## TL;DR

This paper derives exact short-time height distribution formulas for the 1D KPZ equation with Brownian initial conditions, revealing detailed large deviation behaviors and phase transition features.

## Contribution

It provides the first exact expressions for the rate function of the KPZ height distribution with Brownian initial conditions, connecting to weak noise theory and symmetry breaking phenomena.

## Key findings

- Exact rate function $\Phi(H)$ for $H<H_{c2}$ derived.
- Identified phase transition point $H_{c2}$ with symmetry breaking.
- Asymmetric tails with $|H|^{5/2}$ and $H^{3/2}$ behavior.

## Abstract

The early time regime of the Kardar-Parisi-Zhang (KPZ) equation in $1+1$ dimension, starting from a Brownian initial condition with a drift $w$, is studied using the exact Fredholm determinant representation. For large drift we recover the exact results for the droplet initial condition, whereas a vanishingly small drift describes the stationary KPZ case, recently studied by weak noise theory (WNT). We show that for short time $t$, the probability distribution $P(H,t)$ of the height $H$ at a given point takes the large deviation form $P(H,t) \sim \exp{\left(-\Phi(H)/\sqrt{t} \right)}$. We obtain the exact expressions for the rate function $\Phi(H)$ for $H<H_{c2}$. Our exact expression for $H_{c2}$ numerically coincides with the value at which WNT was found to exhibit a spontaneous reflection symmetry breaking. We propose two continuations for $H>H_{c2}$, which apparently correspond to the symmetric and asymmetric WNT solutions. The rate function $\Phi(H)$ is Gaussian in the center, while it has asymmetric tails, $|H|^{5/2}$ on the negative $H$ side and $H^{3/2}$ on the positive $H$ side.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1705.04654/full.md

## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1705.04654/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1705.04654/full.md

---
Source: https://tomesphere.com/paper/1705.04654