Superfluid helium ultralight dark matter detector

dc.contributor.authorHirschel, M.
dc.contributor.authorVadakkumbatt, V.
dc.contributor.authorBaker, N. P.
dc.contributor.authorSchweizer, F. M.
dc.contributor.authorSankey, J. C.
dc.contributor.authorSingh, S.
dc.contributor.authorDavis, J. P.
dc.date.accessioned2024-07-01T19:18:51Z
dc.date.available2024-07-01T19:18:51Z
dc.date.issued2024-05-10
dc.descriptionThis 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
dc.description.abstractThe 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.
dc.description.sponsorshipThe authors would like to thank Samy Boutros, Kripa Vyas, and Brigitte Vachon for fruitful discussions. They acknowledge that the land on which this work was performed is in Treaty Six Territory, the traditional territories of many First Nations, Métis, and Inuit in Alberta. Moreover, they acknowledge support from the University of Alberta; the Natural Sciences and Engineering Research Council, Canada (Grants No. RGPIN-2022-03078 and No. CREATE-495446-17); the Arthur B. McDonald Canadian Astroparticle Physics Research Institute through the support of the Canada First Research Excellence Fund; the National Science Foundation Grants No. PHY-1912480 and No. PHY-2047707; and the Office of the Under Secretary of Defense for Research and Engineering under Grant No. FA9550-22-1-0323.
dc.identifier.citationHirschel, 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.
dc.identifier.issn2470-0029
dc.identifier.urihttps://udspace.udel.edu/handle/19716/34549
dc.language.isoen_US
dc.publisherPhysical Review D
dc.titleSuperfluid helium ultralight dark matter detector
dc.typeArticle

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