R. Geiger
PSL Research University
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Publication
Featured researches published by R. Geiger.
Physical Review Letters | 2016
I. Dutta; Denis Savoie; Bess Fang; B. Venon; C. L. Garrido Alzar; R. Geiger; A. Landragin
We report the operation of a cold-atom inertial sensor which continuously captures the rotation signal. Using a joint interrogation scheme, where we simultaneously prepare a cold-atom source and operate an atom interferometer (AI), enables us to eliminate the dead times. We show that such continuous operation improves the short-term sensitivity of AIs, and demonstrate a rotation sensitivity of 100u2009u2009nrad/sec/sqrt[Hz] in a cold-atom gyroscope of 11u2009u2009cm^{2} Sagnac area. We also demonstrate a rotation stability of 1u2009u2009nrad/sec at 10^{4}u2009u2009sec of integration time, which represents the state of the art for atomic gyroscopes. The continuous operation of cold-atom inertial sensors will lead to large area AIs at their full sensitivity potential, determined by the quantum noise limit.
Physical Review D | 2016
Walid Chaibi; R. Geiger; B. Canuel; Andrea Bertoldi; A. Landragin; Philippe Bouyer
We propose a new detection strategy for gravitational waves (GWs) below few Hertz based on a correlated array of atom interferometers (AIs). nOur proposal allows to reject the Newtonian Noise (NN) which limits all ground based GW detectors below few Hertz, including previous atom interferometry-based concepts. nUsing an array of long baseline AI gradiometers yields several estimations of the NN, whose effect can thus be reduced via statistical averaging. nConsidering the km baseline of current optical detectors, a NN rejection of factor 2 could be achieved, and tested with existing AI array geometries. nExploiting the correlation properties of the gravity acceleration noise, we show that a 10-fold or more NN rejection is possible with a dedicated configuration. nConsidering a conservative NN model and the current developments in cold atom technology, we show that strain sensitivities below
Physical Review A | 2014
M. Meunier; I. Dutta; R. Geiger; C. Guerlin; C. L. Garrido Alzar; A. Landragin
1times 10^{-19}/sqrt{Hz}
arXiv: Atomic Physics | 2016
Bess Fang; I. Dutta; Pierre Gillot; Denis Savoie; J. Lautier; Bing Cheng; C. L. Garrido Alzar; R. Geiger; S. Merlet; F. Pereira Dos Santos; A. Landragin
in the
Journal of Physics B | 2017
Isabelle Riou; Nicolas Mielec; Grégoire Lefèvre; M. Prevedelli; A. Landragin; Philippe Bouyer; Andrea Bertoldi; R. Geiger; B. Canuel
0.3-3 Hz
international frequency control symposium | 2017
D. Savoie; M. Altorio; B. Fang; R. Geiger; A. Landragin
frequency band can be within reach, with a peak sensitivity of
european quantum electronics conference | 2017
Nicolas Mielec; Sapam Ranjita Chanu; Isabelle Riou; B. Canuel; D. Holleville; Bess Fang; A. Landragin; R. Geiger
3times 10^{-23} /sqrt{Hz}
International Conference on Space Optics 2016 | 2017
Isabelle Riou; G. Lefèvre; Nicolas Mielec; Louis Amand; R. Geiger; S. Pelisson; Andrea Bertoldi; B. Canuel; Philippe Bouyer; A. Landragin; Nikos Karafolas; Bruno Cugny; Zoran Sodnik
at
arXiv: Atomic Physics | 2018
Denis Savoie; A. Landragin; R. Geiger; M. Altorio; L.A. Sidorenkov; Bess Fang
2 Hz
european quantum electronics conference | 2017
B. Fang; D. Savoie; Nicolas Mielec; I. Dutta; B. Venon; C. L. Garrido Alzar; R. Geiger; A. Landragin
. nOur proposed configuration could extend the observation window of current detectors by a decade and fill the gap between nground-based and space-based instruments.