2018
DOI: 10.1088/1367-2630/aaf07d
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Improving the accuracy of atom interferometers with ultracold sources

Abstract: We report on the implementation of ultracold atoms as a source in a state of the art atom gravimeter. We perform gravity measurements with 10nm s −2 statistical uncertainties in a so-far largely unexplored temperature range for such a high accuracy sensor, down to 50 nK. This allows for an improved characterization of the most limiting systematic effect, related to wavefront aberrations of light beamsplitters. A thorough model of the impact of this effect onto the measurement is developed and a method is prop… Show more

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Cited by 95 publications
(90 citation statements)
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References 43 publications
(66 reference statements)
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“…Changes in the mean atomic trajectory or temperature then lead to a limitation of the stability of the sensors. Wavefront aberrations coupled to the transverse expansion of the atom cloud in the laser beam is, for example, a limiting factor to the accuracy of cold-atom gravimeters [1-3] and has pointed towards using ultra-cold atom sources for improved accuracy [4]. Even in differential configurations such as used in atomic gyroscopes with counter-propagating atom clouds [5][6][7][8], in gravity gradiometry [9] or gravitational wave detectors [10], stochastic variations of the atom trajectories or of the laser field wavefront pose severe constraints on the optics and on the temperature and initial position jitter of the atom source.…”
Section: Introductionmentioning
confidence: 99%
“…Changes in the mean atomic trajectory or temperature then lead to a limitation of the stability of the sensors. Wavefront aberrations coupled to the transverse expansion of the atom cloud in the laser beam is, for example, a limiting factor to the accuracy of cold-atom gravimeters [1-3] and has pointed towards using ultra-cold atom sources for improved accuracy [4]. Even in differential configurations such as used in atomic gyroscopes with counter-propagating atom clouds [5][6][7][8], in gravity gradiometry [9] or gravitational wave detectors [10], stochastic variations of the atom trajectories or of the laser field wavefront pose severe constraints on the optics and on the temperature and initial position jitter of the atom source.…”
Section: Introductionmentioning
confidence: 99%
“…To meet these stringent requirements, the temperatures of the atomic ensembles have to be drastically reduced (down to a sub-nK level) and their size must remain compact (not exceeding a few mm after several seconds of free expansion) clearly indicating the necessity of using Bose-Einstein Condensates (BEC). Such a direction is taken by several metrology groups worldwide [4][5][6][7][8][9][10] , including the QUANTUS and MAIUS consortia 11 which reached important milestones in controlling quantum gases dynamics in microgravity conditions using atom chips 12,13 .…”
Section: Introductionmentioning
confidence: 99%
“…A modest beam pick off from Raman 1 is sent from module (f) to module (b). This module creates the repump light sent to the 3D MOT module (c) but also the outputs (13) and (14) used for preparation and detection.…”
Section: Micro-optic Modulesmentioning
confidence: 99%