2021
DOI: 10.1038/s41598-021-95334-7
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Multi-loop atomic Sagnac interferometry

Abstract: The sensitivity of light and matter-wave interferometers to rotations is based on the Sagnac effect and increases with the area enclosed by the interferometer. In the case of light, the latter can be enlarged by forming multiple fibre loops, whereas the equivalent for matter-wave interferometers remains an experimental challenge. We present a concept for a multi-loop atom interferometer with a scalable area formed by light pulses. Our method will offer sensitivities as high as $$2\times 10^{-11}$$ … Show more

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Cited by 20 publications
(12 citation statements)
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References 82 publications
(151 reference statements)
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“…Note that the initial mean atomic density at a s = 1.7a 0 is estimated as 2.9E13 − 4.5E13 /cm 3 , depending on the initial loading condition. The mirror pulse efficiency 1 − b has the highest value at a s < 6a 0 , and gradually reduces at larger a s because of the enlarged interaction-induced momentum width [15,22,23]. Note that the initial center-of-mass momentum also degrades the mirror efficiency but the theoretical upper bound for our case is 99.98%, which is negligible degradation.…”
Section: Scaling Behavior Of Cold Collisionsmentioning
confidence: 61%
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“…Note that the initial mean atomic density at a s = 1.7a 0 is estimated as 2.9E13 − 4.5E13 /cm 3 , depending on the initial loading condition. The mirror pulse efficiency 1 − b has the highest value at a s < 6a 0 , and gradually reduces at larger a s because of the enlarged interaction-induced momentum width [15,22,23]. Note that the initial center-of-mass momentum also degrades the mirror efficiency but the theoretical upper bound for our case is 99.98%, which is negligible degradation.…”
Section: Scaling Behavior Of Cold Collisionsmentioning
confidence: 61%
“…We have also demonstrated quantum lock-in amplification [18]. The system may be useful for multiple-loop Sagnac interferometry [15], for noise spectrum analysis [35] and, perhaps, for resonant detection of gravitational waves [41].…”
mentioning
confidence: 95%
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“…Furthermore, freespace cold atom interferometers are currently quite large, heavy, consume significant power, are expensive, and are technologically complex [5]. However, a new multi-loop concept which can significantly improve the performance of free-space interferometers was recently proposed [11].…”
Section: Introductionmentioning
confidence: 99%