Journal
PHYSICAL REVIEW A
Volume 82, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevA.82.043624
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Funding
- Israel Science Foundation [582/07]
- United States-Israel Binational Science Foundation (BSF) [2008141]
- National Science Foundation through Institute for Theoretical Atomic, Molecular, and Optical Physics at Harvard University
- Smithsonian Astrophysical Observatory
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We optimize the signal-to-noise ratio of a Mach-Zehnder atom interferometer with Gaussian squeezed input states in the presence interactions. For weak interactions, our results coincide with those of Huang and Moore [Y. P. Huang and M. G. Moore, Phys. Rev. Lett. 100, 250406 (2008)], with an optimal initial number variance sigma(o) alpha N-1/3 and an optimal signal-to-noise ratio s(o) alpha N-2/3 for the total atom number N. As the interaction strength u increases past unity, phase diffusion becomes dominant, leading to a transition in the optimal squeezing from initial number squeezing to initial phase squeezing with sigma(o) alpha root uN and s(o) alpha root N/u shot-noise scaling. The initial phase squeezing translates into hold-time number squeezing, which is less sensitive to interactions than coherent states and improves so by a factor of root u.
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