The Sagnac effect, manifest in the phase shift of a rotating interferometer proportional to its physical area and to the rotation rate of the frame, plays a crucial role in modern physics being generalized to any kind of interferometer. However, as compared to light, the accurate experimental validation of the Sagnac effect for matter-waves remains challenging. We report the accurate measurement of the Sagnac phase shift, induced by the Earth’s rotation, using a large-area cold atom interferometer. We probe the atomic Sagnac phase shift along the two orthogonal horizontal axes in various orientation of the sensor with respect to geographic north and obtain an agreement with the theoretical prediction at the 20 ppm level, improving by twenty five-fold over the previous achievements for matter waves. Our results underline the universality of the Sagnac effect and open new horizons for testing other fundamental theories, as well as for a number of technological applications in seismology, geodesy and inertial navigation systems.
This presentation will review some of the latest state-of-the-art developments in cold-atom inertial sensors developped at the SYRTE laboratory in Paris.
During the past decades, atom interferometry experiments were developed for various applications like precision measurement of fundamental constants [1, 2], gravimetry [3], gradiometry [4] or inertial sensing [5, 6].
KEYWORDS: Quantum optics, Current controlled current source, Interferometers, Gyroscopes, Sensors, Interferometry, Geophysics, Color centers, Inertial navigation systems
We report the first operation of a cold atom inertial sensor without dead time. Dead times in conventional cold atom interferometers originate from the preparation of a cold atom source prior to its injection in the interferometer and where information on inertial signals is lost. We use a sequence where we simultaneously prepare a cold atom source and operate a light pulse atom interferometer to circumvent the dead time limitation. Therefore the sensor continuously captures all the dynamics with respect to an inertial frame. We show that the continuous operation does not degrade the sensitivity and stability of the atom interferometer, by demonstrating a rotation sensitivity level of less than 1 nrad/s after 10 000 s of integration time. Such a sensitivity level improves previous results by more than an order of magnitude and opens applications of cold atom gyroscopes in inertial navigation and geophysics.
B. Canuel, S. Pelisson, L. Amand, A. Bertoldi, E. Cormier, B. Fang, S. Gaffet, R. Geiger, J. Harms, D. Holleville, A. Landragin, G. Lefèvre, J. Lhermite, N. Mielec, M. Prevedelli, I. Riou, P. Bouyer
The Matter-Wave laser Interferometer Gravitation Antenna, MIGA, will be a hybrid instrument composed of a network of atom interferometers horizontally aligned and interrogated by the resonant field of an optical cavity. This detector will provide measurements of sub Hertz variations of the gravitational strain tensor. MIGA will bring new methods for geophysics for the characterization of spatial and temporal variations of the local gravity field and will also be a demonstrator for future low frequency Gravitational Wave (GW) detections. MIGA will enable a better understanding of the coupling at low frequency between these different signals. The detector will be installed underground in Rustrel (FR), at the “Laboratoire Souterrain Bas Bruit” (LSBB), a facility with exceptionally low environmental noise and located far away from major sources of anthropogenic disturbances. We give in this paper an overview of the operating mode and status of the instrument before detailing simulations of the gravitational background noise at the MIGA installation site.
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