TY - GEN
T1 - Optically trapped atom interferometry using the clock transition of large rubidium-87 bose-einstein condensates
AU - McDonald, G.
AU - Altin, P. A.
AU - Döring, D.
AU - Debs, J. E.
AU - Barter, T. H.
AU - Close, J. D.
AU - Robins, N. P.
AU - Haine, S. A.
AU - Hanna, T. M.
AU - Anderson, R. P.
PY - 2011
Y1 - 2011
N2 - We present a Ramsey-type atom interferometer operating with an optically trapped sample of 106 Bose-condensed 87Rb atoms. We investigate this interferometer experimentally and theoretically with an eye to the construction of future high precision atomic sensors. Our results indicate that, with further experimental refinements, it will be possible to produce and measure the output of a sub-shot-noise limited, large atom number BEC-based interferometer. The optical trap (shown in Figure 1 (c)) allows us to couple the |F = 1,mF = 0) → |F = 2,mF = 0) clock states using a single photon 6.8 GHz microwave transition, while state selective readout is achieved with absorption imaging. We analyse the process of absorption imaging and show that it is possible to observe atom number variance directly, with a signal-to-noise ratio ten times better than the atomic projection noise limit on 106 condensate atoms. We discuss the technical and fundamental noise sources that limit our current system, and present theoretical and experimental results on interferometer contrast, de-phasing and miscibility.
AB - We present a Ramsey-type atom interferometer operating with an optically trapped sample of 106 Bose-condensed 87Rb atoms. We investigate this interferometer experimentally and theoretically with an eye to the construction of future high precision atomic sensors. Our results indicate that, with further experimental refinements, it will be possible to produce and measure the output of a sub-shot-noise limited, large atom number BEC-based interferometer. The optical trap (shown in Figure 1 (c)) allows us to couple the |F = 1,mF = 0) → |F = 2,mF = 0) clock states using a single photon 6.8 GHz microwave transition, while state selective readout is achieved with absorption imaging. We analyse the process of absorption imaging and show that it is possible to observe atom number variance directly, with a signal-to-noise ratio ten times better than the atomic projection noise limit on 106 condensate atoms. We discuss the technical and fundamental noise sources that limit our current system, and present theoretical and experimental results on interferometer contrast, de-phasing and miscibility.
UR - http://www.scopus.com/inward/record.url?scp=84893579843&partnerID=8YFLogxK
UR - https://arxiv.org/pdf/1011.4713
M3 - Conference contribution
SN - 9780977565771
T3 - Optics InfoBase Conference Papers
SP - 116
EP - 118
BT - Conference on Lasers and Electro-Optics/Pacific Rim, CLEOPR 2011
T2 - Conference on Lasers and Electro-Optics/Pacific Rim, CLEOPR 2011
Y2 - 28 August 2011 through 1 September 2011
ER -