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arxiv: 1403.3485 · v2 · pith:V3NU2FJGnew · submitted 2014-03-14 · 🪐 quant-ph · cond-mat.quant-gas· nlin.PS

A Bright Solitonic Matter-Wave Interferometer

classification 🪐 quant-ph cond-mat.quant-gasnlin.PS
keywords wavesolitonicinterferometermatteratomsattractivebrightcompared
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We present the first realisation of a solitonic atom interferometer. A Bose-Einstein condensate of $1\times10^4$ atoms of rubidium-85 is loaded into a horizontal optical waveguide. Through the use of a Feshbach resonance, the $s$-wave scattering length of the $^{85}$Rb atoms is tuned to a small negative value. This attractive atomic interaction then balances the inherent matter-wave dispersion, creating a bright solitonic matter wave. A Mach-Zehnder interferometer is constructed by driving Bragg transitions with the use of an optical lattice co-linear with the waveguide. Matter wave propagation and interferometric fringe visibility are compared across a range of $s$-wave scattering values including repulsive, attractive and non-interacting values. The solitonic matter wave is found to significantly increase fringe visibility even compared with a non-interacting cloud.

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