Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

Viewpoint: Optical Quantum Logic at the Ultimate Limit

A. S. Parkins

Published Nov 7, 2016• 0 citations
OpenAlex

Abstract

Microscopic clouds of cold atoms can mediate interactions between weak pulses of light at the level required for quantum logic with single photons.

Related papers

Quantum logic using photon-exchange interactions

J. D. Franson, T. B. Pittman

Nonlinear optical effects at the two-photon level are usually negligible because of the weak electric field associated with a single photon.

Quantum Electronics and Laser Science Conference•May 1, 2000•0 citations

Optical Quantum Logic at the Ultimate Limit

A. S. Parkins

Physics•Nov 7, 2016•3 citations

SWITCHING OF LIGHT WITH LIGHT USING COLD ATOMS INSIDE A HOLLOW OPTICAL FIBER

Michal Bajcsy, Sebastian Hofferberth, Thibault Peyronel +5 more

We demonstrate a fiber-optical switch that operates with a few hundred photons per switching pulse. The light-light interaction is mediated by laser-cooled atoms. The required strong interaction between atoms and light is achieved by simultaneously confining photons and atoms inside the microscopic hollow core of a single-mode photonic-crystal fiber.

Laser Spectroscopy•Feb 1, 2010•0 citations

Switching Light by Vacuum

Michael Fleischhauer

An opaque cloud of cold atoms becomes transparent when a few photons occupy an empty cavity, creating an optical switch for processing quantum information.

Science•Sep 1, 2011•4 citations

WGQED1D: a microscopic N-atom waveguide-QED toolkit for single-photon scattering and weak-measurement experiments

Mauricio Herrera

Abstract We present \code{WGQED1D}, a lightweight, validated Python toolkit for microscopic simulation of single-photon scattering by $N$ two-level atoms in a one-dimensional bidirectional waveguide. The toolkit implements the standard non-Hermitian effective Hamiltonian on the single-excitation manifold, with bidirectional dipole--dipole interactions mediated by retarded photon exchange, together with the input--output relation needed to reconstruct the output field. A careful microscopic calibration $\beta = \mathrm{OD}/(2N)$ between optical depth and per-atom waveguide-coupling efficiency is required for quantitative agreement with the free-space Beer--Lambert limit; we verify this calibration to better than $0.1\%$ on a representative range of optical depths. The implementation is deterministic in the single-excitation subspace, runs in $\mathcal{O}(N^2)$ memory and $\mathcal{O}(N^2)$ operations per timestep, and produces converged results for realistic atomic ensembles ($N\sim 200$--$1000$) in seconds to minutes on a laptop. We document the model, implementation, and three validations: (i) pulse-averaged Beer--Lambert transmission across $\OD\in[0.25,3]$; (ii) the Wiseman--Steinberg weak-value formula $\tauT = \langle\tauG\rangle_{\rm post}$ for the post-selected atomic excitation time; and (iii) direct comparison with recent experimental data from the Angulo et al.\ measurement of negative atomic excitation time [Phys.\ Rev.\ Lett.\ \textbf{136}, 153601 (2026)]. The toolkit provides a reproducible numerical platform for studies of weak measurement, anomalous dispersion, group delay, and post-selected observables in single-photon transmission through optically thick atomic clouds. The source code is openly available under the MIT license.

•Jul 21, 2026•0 citations

Room for Just One Photon

Philippe Grangier

Ensembles of cold atoms excited up to Rydberg states can be used to manipulate and control interactions between single photons.

Science•May 17, 2012•2 citations
Abstract We present \code{WGQED1D}, a lightweight, validated Python toolkit for microscopic simulation of single-photon scattering by NNN two-level atoms in a one-dimensional bidirectional waveguide. The toolkit implements the standard non-Hermitian effective Hamiltonian on the single-excitation manifold, with bidirectional dipole--dipole interactions mediated by retarded photon exchange, together with the input--output relation needed to reconstruct the output field. A careful microscopic calibration β=OD/(2N)\beta = \mathrm{OD}/(2N)β=OD/(2N) between optical depth and per-atom waveguide-coupling efficiency is required for quantitative agreement with the free-space Beer--Lambert limit; we verify this calibration to better than 0.1%0.1\%0.1% on a representative range of optical depths. The implementation is deterministic in the single-excitation subspace, runs in O(N2)\mathcal{O}(N^2)O(N2) memory and O(N2)\mathcal{O}(N^2)O(N2) operations per timestep, and produces converged results for realistic atomic ensembles (N∼200N\sim 200N∼200--100010001000) in seconds to minutes on a laptop. We document the model, implementation, and three validations: (i) pulse-averaged Beer--Lambert transmission across $\OD\in[0.25,3]$; (ii) the Wiseman--Steinberg weak-value formula $\tauT = \langle\tauG\rangle_{\rm post}$ for the post-selected atomic excitation time; and (iii) direct comparison with recent experimental data from the Angulo et al.\ measurement of negative atomic excitation time [Phys.\ Rev.\ Lett.\ \textbf{136}, 153601 (2026)]. The toolkit provides a reproducible numerical platform for studies of weak measurement, anomalous dispersion, group delay, and post-selected observables in single-photon transmission through optically thick atomic clouds. The source code is openly available under the MIT license.