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arxiv: 2411.19807 · v2 · pith:CKX2DNA5new · submitted 2024-11-29 · ❄️ cond-mat.quant-gas · physics.atom-ph

The Rayleigh-Taylor instability in a binary quantum fluid

classification ❄️ cond-mat.quant-gas physics.atom-ph
keywords instabilityinterfacebinaryfluidfluidsimmisciblequantumrayleigh-taylor
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Instabilities, where small fluctuations seed the formation of large-scale structures, govern dynamics in a variety of fluid systems. The Rayleigh-Taylor instability (RTI), present from tabletop to astronomical scales, is an iconic example characterized by mushroom-shaped incursions appearing when immiscible fluids are forced together. Despite its ubiquity, RTI experiments are challenging; here, we report the observation of the RTI in an immiscible binary superfluid consisting of a two-component Bose-Einstein condensate. We force these components together to initiate the instability, and observe the growth of mushroom-like structures. The interface can also be stabilized, allowing us to spectroscopically measure the "ripplon" interface modes. Lastly, we use matter-wave interferometry to transform the superfluid velocity field at the interface into a vortex chain. These results-in agreement with our theory-demonstrate the close connection between the RTI in classical and quantum fluids.

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