Mattewaves are promising candidates for the realization of extremely sensitive sensors. Some of the most sensitive and precise measurements to date of gravity [1], inertia [2], and rotation [3] are based on matter-wave interferometry with free-falling atomic clouds. A critical requirement to achieve very high sensitivities is the long interrogation time, which consequently leads to experimental apparatus up to a hundred meters tall or the requirement for experiments to be performed in microgravity in space[4–7]. To tackle this problem, the gravitational acceleration must be cancelled, e.g. by manipulating atomic waves in time-changeable traps and waveguides [8]. In the past, we demonstrated near-perfect smooth and controllable matter- wave guides by transporting Bose-Einstein condensates (BECs) over macroscopic distances without any heating or decohering their internal quantum states [9]. A neutral-atom accelerator ring was utilized to bring BECs to very high speeds (up to 16 times their sound velocity) and transport them in a magnetic matter-wave guide for 15 centimetres whilst fully preserving their internal coherence.
If this represents a ‘perfect’ waveguide then what is a non-perfect waveguide? How much imperfection can a waveguide tolerate before it starts to harm quantum-transport? In this presentation, we will introduce the basics of TAAP waveguides and explore experimentally how strong an obstacle has to be in order to disturb the travelling matterwave. We propose a simple fundamental limit which depends only on the transverse trapping frequencies.
References
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