
TL;DR
This paper links non-Hermitian physics to spacetime geometry, showing how curvature gradients induce gain, loss, and skin effects, unifying these phenomena within a geometric framework.
Contribution
It introduces a metric-based approach to understanding non-Hermitian effects, revealing how spacetime deformations produce physical NH phenomena like gain, loss, and skin effects.
Findings
Pseudo-Hermitian Hamiltonians arise in static, diagonal coordinates ensuring real spectra.
Time-dependent coordinates break pseudo-Hermiticity, leading to nonunitary evolution.
Space-dependent coordinates cause the non-Hermitian skin effect, localizing states at boundaries.
Abstract
I consider the longstanding issue of the hermiticity of the Dirac equation in curved spacetime. Instead of imposing hermiticity by adding ad hoc terms, I renormalize the field by a scaling function, which is related to the determinant of the metric, and then regularize the renormalized field on a discrete lattice. I found that, for time-independent and diagonal (or conformally flat) coordinates, the Dirac equation returns a pseudo-Hermitian (i.e., PT-symmetric) Hamiltonian when properly regularized on the lattice. Notably, the PT-symmetry is unbroken, ensuring a real energy spectrum and unitary time evolution. This establishes stringent conditions for the existence of complex spectra in 1D non-Hermitian (NH) models. Conversely, time-dependent spacetime coordinates break pseudohermiticity, yielding NH Hamiltonians with nonunitary time evolution. Similarly, space-dependent coordinates…
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