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We show that light-pulse atom interferometry with atomic point sources and spatially resolved detection enables multi-axis (two rotation, one acceleration) precision inertial sensing at long interrogation times.
C. Monroe, W. Swann, H. Robinson, and C. Wieman, Physical Review Letters 65
1990
Earlier work this paper cites.
M. Kasevich and S. Chu, Physical Review Letters 67
1991
Earlier work this paper cites.
J. Audretsch and K.-P. Marzlin, Physical Review A 50
1994
Earlier work this paper cites.
K. B. Davis, M. O. Mewes, M. R. Andrews, N. van Druten, D. Durfee, D. Kurn, and W. Ketterle, Physical Review Letters 75
1995
Earlier work this paper cites.
T. L. Gustavson, P. Bouyer, and M. A. Kasevich, Physical Review Letters 78
1997
Earlier work this paper cites.
H. Ammann and N. Christensen, Physical Review Letters 78
1997
Earlier work this paper cites.
A. Peters, K. Y. Chung, and S. Chu, Metrologia 38
2001
Earlier work this paper cites.
J. H. Denschlag, J. E. Simsarian, H. Häffner, C. McKenzie, A. Browaeys, D. Cho, K. Helmerson, S. L. Rolston, and W. D. Phillips, Journal of Physics B: Atomic, Molecular and Optical Physics 35
2002
Cited alongside, same era.
G. T. Foster, J. B. Fixler, J. M. McGuirk, and M. A. Kasevich, Optics Letters 27
2002
Cited alongside, same era.
J. B. Fixler, G. T. Foster, J. M. McGuirk, and M. A. Kasevich, Science 315
2007
Cited alongside, same era.
S. Dimopoulos, P. W. Graham, J. M. Hogan, and M. A. Kasevich, Physical Review D 78
2008
Cited alongside, same era.
H. Müller, S.-w. Chiow, S. Herrmann, S. Chu, and K.-Y. Chung, Physical Review Letters 100
2008
Cited alongside, same era.
R. Bouchendira, P. Cladé, S. Guellati-Khélifa, F. Nez, and F. Biraben, Physical Review Letters 106
2011
Later among the works it cites.
J. M. Hogan, D. M. S. Johnson, S. Dickerson, T. Kovachy, A. Sugarbaker, S.-w. Chiow, P. W. Graham, M. A. Kasevich, B. Saif, S. Rajendran, P. Bouyer, B. D. Seery, L. Feinberg, and R. Keski-Kuha, General Relativity and Gravitation 43
2011
Later among the works it cites.
R. Dubessy, K. Merloti, L. Longchambon, P.-E. Pottie, T. Liennard, A. Perrin, V. Lorent, and H. Perrin, Physical Review A 85
2012
Later among the works it cites.
S. Dickerson, J. M. Hogan, D. M. S. Johnson, T. Kovachy, A. Sugarbaker, S.-w. Chiow, and M. A. Kasevich, The Review of Scientific Instruments 83
2012
Later among the works it cites.
S.-Y. Lan, P.-C. Kuan, B. Estey, P. Haslinger, and H. Müller, Physical Review Letters 108
2012
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2009
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S. R. Segal, Q. Diot, E. A. Cornell, A. A. Zozulya, and D. Z. Anderson, Physical Review A 81
2010
Cited alongside, same era.
See Supplemental Material (in arXiv ancillary files) for further description of Principal Component Analysis and its use in finding spatial fringe contrast
Cited in the paper.
The procedure is similar in principle to δ \delta -kick cooling [ 24 ] , but uses the atoms’ continuous expansion over ∼ 100 m s \sim 100\text{m}\text{s} against a shallow ( ∼ 5 Hz \sim 5\text{Hz} ) harmonic trap [ 25 ] rather than a short (few ms) impulse [ 7 ] . The magnetic fields are rapidly turned off when the atoms have reached their minimum velocity (maximum expansion) in all three dimensions
Cited in the paper.
Integrated contrast is calculated by summing image counts inside regions of interest around each output port and then forming the normalized population ratios r i r_{i} for a set. The contrast of the set is c = [ Max ( r i ) − Min ( r i ) ] / [ Max ( r i ) + Min ( r i ) ] c=[\text{Max}(r_{i})-\text{Min}(r_{i})]/[\text{Max}(r_{i})+\text{Min}(r_{i})]
Cited in the paper.
To ensure that results are independent of the initial grid registration, we compute two grid alignment quadratures (analogous to sine and cosine) for each dimension by offsetting the grid by s / 2 s/2 in each direction. We then average over alignment using the root mean square of these four results
Cited in the paper.
The sensitivity is δ a / g = δ ϕ / k eff g T 2 \delta a/g=\delta\phi/k_{\text{eff}}gT^{2} , where δ ϕ = ( 2.0 m rad ) / 2 \delta\phi=(2.0~\text{m}\text{rad})/\sqrt{2} is the absolute phase noise combining all the atoms from both the even and odd grid squares
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H. Müntinga, H. Ahlers, M. Krutzik, A. Wenzlawski, S. Arnold, D. Becker, K. Bongs, H. Dittus, H. Duncker, N. Gaaloul, C. Gherasim, E. Giese, C. Grzeschik, T. W. Hänsch, O. Hellmig, W. Herr, S. Herrmann, E. Kajari, S. Kleinert, C. Lämmerzahl, W. Lewoczko-Adamczyk, J. Malcolm, N. Meyer, R. Nolte, A. Peters, M. Popp, J. Reichel, A. Roura, J. Rudolph, M. Schiemangk, M. Schneider, S. T. Seidel, K. Sengstock, V. Tamma, T. Valenzuela, A. Vogel, R. Walser, T. Wendrich, P. Windpassinger, W. Zeller, T. van Zoest, W. Ertmer, W. P. Schleich, and E. M. Rasel, Physical Review Letters 110
2013
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