In resonant-mode atom-interferometer gravitational wave detectors, the optimal number of pulses is set mainly by per-pulse atom loss, and current large-pulse-number proposals demand fidelities roughly two orders of magnitude beyond the state of the art.
Abendet al., Terrestrial very-long-baseline atom in- terferometry: Workshop summary, A VS Quantum Sci.6, 024701 (2024)
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Spatial and Pulse Efficiency Constraints in Atom Interferometric Gravitational Wave Detectors
In resonant-mode atom-interferometer gravitational wave detectors, the optimal number of pulses is set mainly by per-pulse atom loss, and current large-pulse-number proposals demand fidelities roughly two orders of magnitude beyond the state of the art.