Semiclassical tunneling for some 1D Schrödinger operators with complex-valued potentials
Martin Averseng, Nicolas Frantz, Frédéric Hérau, Nicolas Raymond
TL;DR
This work extends semiclassical tunneling analysis to a non-selfadjoint Schrödinger operator with a complex-valued potential, L(h) = -h^2 d_x^2 + e^{iα}V with V even and possessing two symmetric wells. The authors develop a robust framework combining elliptic estimates, Agmon localization, and WKB constructions to reduce spectral analysis to the left and right wells and to a complex harmonic oscillator model. They demonstrate that the low-energy spectrum near the origin consists of exponentially close pairs, with gaps governed by an explicit complex tunneling factor S(α) and a prefactor A, while all other spectrum remains separated by a larger O(h) scale; for α ≠ 0 the pair exhibits a characteristic rotation in the complex plane. The analysis yields a precise asymptotic description of the eigenvalue gap and the associated quasi-modes, providing a rigorous extension of the standard HS84-type tunneling results to non-selfadjoint settings with complex potentials. This has implications for understanding tunneling and decay for non-selfadjoint quantum systems and related PDEs in the semiclassical regime.
Abstract
We consider the non-selfadjoint, semiclassical Schrödinger operator $\mathscr{L}(h) := -h^2\partial_x^2+e^{iα}V$, where $α\in (-π,π)$ and $V: \mathbb{R}\to \mathbb{R}_+$ is even and vanishes at exactly two (symmetric) non-degenerate minima. We establish a semiclassical tunneling result: the spectrum of $\mathscr{L}(h)$ near the origin is given by a sequence of algebraically simple eigenvalues which come in exponentially close pairs (within a $\mathscr{O}(e^{-S/h})$ distance where $S > 0$ is explicit), each pair being separated from the others by a distance $\mathscr{O}(h)$. A one-term estimate of the gap between the two smallest eigenvalues in magnitude is derived; it reveals that, when $α\neq 0$, they quickly rotate around each other as $h$ goes to $0$.
