Optimal baseline exploitation in vertical dark-matter detectors based on atom interferometry
Fabio Di Pumpo, Alexander Friedrich, Enno Giese

TL;DR
This paper determines the optimal configuration for vertical atom interferometry detectors for dark matter and gravitational waves, revealing how baseline length and design choices influence sensitivity limits.
Contribution
It introduces a fundamental sensitivity limit for vertical atom interferometry detectors and compares different configurations, including a novel multi-diamond scheme, to optimize resource use.
Findings
Optimal detector height is 20% of the baseline for maximum sensitivity.
Doubling the baseline reduces measurement uncertainty by about 65%.
Different configurations reach the same fundamental sensitivity limit.
Abstract
Several terrestrial detectors for gravitational waves and dark matter based on long-baseline atom interferometry are currently in the final planning stages or already under construction. These upcoming vertical sensors are inherently subject to gravity and thus feature gradiometer or multi-gradiometer configurations using single-photon transitions for large momentum transfer. While there has been significant progress on optimizing these experiments against detrimental noise sources and for deployment at their projected sites, finding optimal configurations that make the best use of the available resources are still an open issue. Even more, the fundamental limit of the device's sensitivity is still missing. Here we fill this gap and show that (a) resonant-mode detectors based on multi-diamond fountain gradiometers achieve the optimal, shot-noise limited, sensitivity if their height…
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Taxonomy
TopicsCold Atom Physics and Bose-Einstein Condensates · Advanced Frequency and Time Standards · Atomic and Subatomic Physics Research
