# Topological Bounds for Fourier Coefficients and Applications to Torsion

**Authors:** Stefan Steinerberger

arXiv: 1705.02651 · 2017-10-10

## TL;DR

This paper establishes topological bounds on Fourier coefficients related to convex domain PDEs, revealing how the geometry of the domain influences the spectral properties of solutions and their derivatives.

## Contribution

It introduces a novel topological bound for Fourier coefficients based on sign changes, linking domain geometry to spectral gaps and derivative estimates of harmonic functions.

## Key findings

- Bound on the spectral gap of the Hessian at the maximum point of the solution.
- Fourier coefficient bounds depending on the number of sign changes of functions.
- Implications for decay rates of solutions to the heat equation.

## Abstract

Let $\Omega \subset \mathbb{R}^2$ be a bounded convex domain in the plane and consider \begin{align*}   -\Delta u &=1 \qquad \mbox{in}~\Omega \\ u &= 0 \qquad \mbox{on}~\partial \Omega. \end{align*} If $u$ assumes its maximum in $x_0 \in \Omega$, then the eccentricity of level sets close to the maximum is determined by the Hessian $D^2u(x_0)$. We prove that $D^2u(x_0)$ is negative definite and give a quantitative bound on the spectral gap $$ \lambda_{\max}\left(D^2u(x_0)\right) \leq - c_1\exp\left( -c_2\frac{diam(\Omega)}{inrad(\Omega)} \right)$$ for universal $c_1, c_2$ This is sharp up to constants. The proof is based on a new lower bound for Fourier coefficients whose proof has a topological component: if $f:\mathbb{T} \rightarrow \mathbb{R}$ is continuous and has $n$ sign changes, then $$ \sum_{k=0}^{n/2}{ \left| \left\langle f, \sin{kx} \right\rangle \right| + \left| \left\langle f, \cos{kx} \right\rangle \right| } \gtrsim_n \frac{ | f\|^{n+1}_{L^1(\mathbb{T})}}{ \| f\|^{n }_{L^{\infty}(\mathbb{T})}}.$$ This statement immediately implies estimates on higher derivatives of harmonic functions $u$ in the unit ball: if $u$ is very flat in the origin, then the boundary function $u(\cos{t}, \sin{t}):\mathbb{T} \rightarrow \mathbb{R}$ has to have either large amplitude or many roots. It also implies that the solution of the heat equation starting with $f:\mathbb{T} \rightarrow \mathbb{R}$ cannot decay faster than $\sim\exp(-(\# \mbox{sign changes})^2 t/4)$.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1705.02651/full.md

## References

31 references — full list in the complete paper: https://tomesphere.com/paper/1705.02651/full.md

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Source: https://tomesphere.com/paper/1705.02651