Published September 10, 2024 | Published
Journal Article Open

Coherent collisional decoherence

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Autonomous University of Barcelona

Abstract

We study the decoherence of a system of 𝑁 noninteracting heavy particles (atoms) due to coherent scattering with a background gas. We introduce a framework for computing the induced phase shift and loss of contrast for arbitrary preparations of 𝑁-particle quantum states. We find phase shifts that are inherently (𝑁≥2)-body effects and may be searched for in future experiments. We analyze simple setups, including a two-mode approximation of an interferometer. We study fully entangled 𝑁⁢00⁢𝑁 states, which resemble the correlated positions in a matter interferometer, as well as totally uncorrelated product states that are representative of a typical state in an atom interferometer. We find that the extent to which coherent enhancements increase the rate of decoherence depends on the observable of interest, state preparation, and details of the experimental design. In the context of future ultralow-recoil (e.g., light dark matter) searches with atom interferometers we conclude that (i) there exists a coherently enhanced scattering phase which can be searched for using standard (i.e., contrast/visibility and phase) interferometer observables; (ii) although decoherence rates of one-body observables are not coherently enhanced, a coherently enhanced loss of contrast can still arise from dephasing; and (iii) higher statistical moments (which are immediately accessible in a counting experiment) are coherently enhanced and may offer a new tool with which to probe the soft scattering of otherwise undetectable particles in the laboratory.

Copyright and License

© 2024 American Physical Society.

Acknowledgement

We thank Klaus Hornberger, Duncan O'Dell and John E. Sipe for feedback during the completion of this work. We also thank Daniel Carney for discussions on the validity of the Born approximation and comments on an early version of this paper. We are especially grateful to Kathryn M. Zurek for many stimulating discussions and comments on the paper.

Funding

C.M. is supported by “Ayuda Beatriz Galindo Junior” from the Spanish “Ministerio de Universidades”, Grant No. BG22/00155. C.M. thanks Caltech for its hospitality during the completion of this work. R.P. and L.B. are supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics under Award No. DE-SC0011632, and by the Walter Burke Institute for Theoretical Physics. R.P. is supported by the Neutrino Theory Network under Award No. DEAC02-07CH11359.

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Additional details

Created:
September 11, 2024
Modified:
November 7, 2024