Non-density of nodal lines in the clamped plate problem
Alberto Enciso, Josef Greilhuber
TL;DR
This work proves that nodal sets of high-frequency clamped plate eigenfunctions need not be dense, by constructing small, symmetry-preserving domain perturbations of the unit disk that admit a high-frequency clamped-plate eigenfunction which remains nonzero in a disk of radius about $0.44$. The strategy hinges on decomposing eigenfunctions into a Helmholtz component $v$ and a non-oscillatory SP component $w$, then carefully perturbing the domain so that $v$ vanishes to high order at the origin while $w$ remains nonzero there; the resulting eigenfunction $u=w-v$ thus preserves a central sign. A combination of Hadamard-type shape derivatives, precise bounds on Bessel functions, and a bespoke one-parameter perturbation yields explicit control over the leading Fourier–Bessel components, allowing a macroscopic nodal void to persist for arbitrarily large frequencies. This demonstrates a qualitative difference from Laplacian eigenfunctions and provides a framework for probing nodal geometry via domain perturbations, with potential implications for spectral geometry of higher-order operators. $\Delta^2 u = \lambda^2 u$ with clamped boundary conditions and the associated shape-derivative analysis are central to achieving explicit, quantitative radii of nodal voids.
Abstract
We show that, in contrast to the case of Laplace eigenfunctions, the nodal set of high energy eigenfunctions of the clamped plate problem is not necessarily dense, and can in fact exhibit macroscopic "nodal voids". Specifically, we show that there are small deformations of the unit disk admitting a clamped plate eigenfunction of arbitrarily high frequency that does not vanish in a disk of radius 0.44.
