Berry's phase on photonic quantum computers
Steven Abel, Iwo Wasek, Simon Williams
TL;DR
This paper develops a CVQC-based protocol to observe Berry's phase for orbital angular momentum in a time-dependent magnetic field, implemented entirely with passive Gaussian operations. By simulating the Hamiltonian $H=\frac{1}{2}\sum_i(p_i^2+q_i^2)-\mu\vec{B}\cdot\vec{L}$ using Strang-Trotter-Suzuki gadgets and a four-mode interferometer, the authors demonstrate that the geometric Berry phase $\gamma(C)$ can be extracted from interferometric readout. They extend the framework to the non-adiabatic regime via the Aharonov-Anandan phase, showing that the averaged phase $\tfrac{1}{2}(\xi_+ + \xi_-)$ tracks $\gamma(C)$ even when dynamical and leading non-geometric contributions are large. The framework is validated both in a quantum emulator (Quandela Perceval) and on the Ascella QPU, confirming experimental feasibility on current photonic hardware and highlighting potential for holonomic and geometric-gate applications in CVQC.
Abstract
We formulate a continuous-variable quantum computing (CVQC) algorithm to study Berry's phase on photonic quantum computers. We demonstrate that CVQC allows the simulation of charged particles with orbital angular momentum under the influence of an adiabatically changing $\vec{B}$ field. Although formulated entirely in the CVQC setting, our construction uses only passive linear-optical operations (beam splitters and phase shifts), which act identically in single-photon photonic architectures. This enables experimental realisation on the Quandella Ascella platform, where we observe the Berry's phase phenomenon with interferometric measurement. We also generalise the framework to more rapid non-adiabatic evolution. By concatenating Aharonov-Anandan cycles for opposing magnetic fields we demonstrate that one can engineer a circuit in which dynamical phases and leading non-geometric errors cancel by symmetry, leaving the intrinsically robust geometric phase contribution.
