Superfluid helium ultralight dark matter detector

Abstract
The absence of a breakthrough in directly observing dark matter (DM) through prominent large-scale detectors motivates the development of novel tabletop experiments probing more exotic regions of the parameter space. If DM contains ultralight bosonic particles, they would behave as a classical wave and could manifest through an oscillating force on baryonic matter that is coherent over ∼106 periods. Our Helium ultraLIght dark matter Optomechanical Sensor (HeLIOS) uses the high-𝑄 acoustic modes of superfluid helium-4 to resonantly amplify this signal. A superconducting reentrant microwave cavity enables sensitive optomechanical readout ultimately limited by thermal motion at millikelvin temperatures. Pressurizing the helium allows for the unique possibility of tuning the mechanical frequency to effectively broaden the DM detection bandwidth. We demonstrate the working principle of our prototype HeLIOS detector and show that future generations of HeLIOS could explore unconstrained parameter space for both scalar and vector ultralight DM after just an hour of integration time.
Description
This article was originally published in Physical Review D . The version of record is available at: https://doi.org/10.1103/PhysRevD.109.095011. © 2024 American Physical Society
Keywords
Citation
Hirschel, M., V. Vadakkumbatt, N. P. Baker, F. M. Schweizer, J. C. Sankey, S. Singh, and J. P. Davis. “Superfluid Helium Ultralight Dark Matter Detector.” Physical Review D 109, no. 9 (May 10, 2024): 095011. https://doi.org/10.1103/PhysRevD.109.095011.