Limits to the sensitivity of a low noise compact atomic gravimeter
By J. L. Gouet, Tanja Mehlstaubler, Jaewan Kim, S. Merlet, A. Clairon, A. Landragin, F. P. D. Santos. 2008
263 citations recorded by the source corpus.
A detailed analysis of the most relevant sources of phase noise in an atomic interferometer is carried out, both theoretically and experimentally. Even a short interrogation time of 100 ms allows our cold atom gravimeter to reach an excellent short term sensitivity to acceleration of 1.4×10-8g at 1 s. This result relies on the combination of a low phase noise laser system, efficient detection scheme and good shielding from vibrations. In particular, we describe a simple and robust technique of vibration compensation, which is based on correcting the interferometer signal by using the ac acceleration signal measured by a low noise seismometer.
Subfields: Atomic and Molecular Physics, and Optics, Statistics and Probability
View Paper: https://www.semanticscholar.org/paper/75095dfbcad14767eb2bc80ecaf4bbeedaf8bddd
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In Atomic and Molecular Physics, and Optics
Citations in the corpus
- STE-QUEST—test of the universality of free fall using cold atom interferometry (2013, background): “Still, the quadratic Zeeman effect coupled to the small offset field B0 = 1 mG and a magnetic field gradient ∇B induce an acceleration [68, 69].”
- Stability comparison of two absolute gravimeters: optical versus atomic interferometers (2014, background): “They are based on the combination of a passive isolation and of a low noise seismometer [4, 15].”
- Atomic Sensors – A Review (2011, unknown): “sensitivities in much smaller instruments [98], [99].”
- The influence of transverse motion within an atomic gravimeter (2011, methodology): “We use the detection scheme tested in the previous prototype [7], which was inspired by the detection system [14] of the gradiometer [15].”
- Precision atomic gravimeter based on Bragg diffraction (2012, methodology): “The precision and accuracy of state-of-the-art atomic gravimeters is presently limited by effects such as Coriolis acceleration and wavefront aberrations [6, 39].”