The Klein-Gordon equation, the Hilbert transform, and dynamics of Gauss-type maps

preprint2020arXivOpen access

Abstract

A pair (Γ,Λ)(Γ,Λ), where Γ⊂R2Γ\subset\mathbb{R}^2 is a locally rectifiable curve and Λ⊂R2Λ\subset\mathbb{R}^2 is a {\em Heisenberg uniqueness pair} if an absolutely continuous (with respect to arc length) finite complex-valued Borel measure supported on ΓΓ whose Fourier transform vanishes on ΛΛ necessarily is the zero measure. Recently, it was shown by Hedenmalm and Montes that if ΓΓ is the hyperbola x1x2=M2/(4π2)x_1x_2=M^2/(4π^2), where M>0M>0 is the mass, and ΛΛ is the lattice-cross (αZ×{0})∪({0}×βZ)(α\mathbb{Z}\times\{0\}) \cup (\{0\}\timesβ\mathbb{Z}), where α,βα,β are positive reals, then (Γ,Λ)(Γ,Λ) is a Heisenberg uniqueness pair if and only if αβM2≤4π2αβM^2\le4π^2. The Fourier transform of a measure supported on a hyperbola solves the one-dimensional Klein-Gordon equation, so the theorem supplies very thin uniqueness sets for a class of solutions to this equation. The case of the semi-axis R+\mathbb{R}_+ as well as the holomorphic counterpart remained open. In this work, we completely solve these two problems. As for the semi-axis, we show that the restriction to R+\mathbb{R}_+ of the above exponential system spans a weak-star dense subspace of L∞(R+)L^\infty(\mathbb{R}_+) if and only if 0<αβ<40<αβ<4, based on dynamics of Gauss-type maps. This has an interpretation in terms of dynamical unique continuation. As for the holomorphic counterpart, we show that the above exponential system with m,n≥0m,n\ge0 spans a weak-star dense subspace of H+∞(R)H^\infty_+(\mathbb{R}) if and only if 0<αβ≤10<αβ\le1. To obtain this result, we need to develop new harmonic analysis tools for the dynamics of Gauss-type maps, related to the Hilbert transform. Some details are deferred to a separate publication.

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