The Rayleigh-Taylor instability in a binary quantum fluid

The Rayleigh-Taylor instability in a binary quantum fluid

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. Last, 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.

The Rayleigh-Taylor instability in a binary quantum fluid; Y. Geng, J. Tao, M. Zhao, S. Mukherjee, S. P. Eckel, G. K. Campbell, and I. B. Spielman; Science Advances 11 eadw9752 (2025). doi:10.1126/sciadv.adw9752; Featured on Science Advances home page.