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    New Constraints on Dark Photon Dark Matter with a Millimeter-Wave Dielectric Haloscope

    Guoqing Wei1,2, Diguang Wu1,2, Runqi Kang1,2, Qingning Jiang1, Man Jiao3,4,5,*, Xing Rong1,2,4,5,†, and Jiangfeng Du4

    • 1Laboratory of Spin Magnetic Resonance, School of Physical Sciences, Anhui Province Key Laboratory of Scientific Instrument Development and Application, University of Science and Technology of China, Hefei 230026, China
    • 2Hefei National Laboratory, University of Science and Technology of China, Hefei 230088, China
    • 3Institute for Advanced Study in Physics and School of Physics, Zhejiang University, Hangzhou 310027, China
    • 4State Key Laboratory of Ocean Sensing and School of Physics, Zhejiang University, Hangzhou 310058, China
    • 5Institute of Quantum Sensing, Institute of Fundamental and Transdisciplinary Research and Zhejiang Key Laboratory of R&D and Application of Cutting-edge Scientific Instruments, Zhejiang University, Hangzhou 310058, China

    • *Contact author: man.jiao@zju.edu.cn
    • †Contact author: xrong@ustc.edu.cn

    Phys. Rev. Lett. 136, 071001 – Published 19 February, 2026

    DOI: https://doi.org/10.1103/yk7n-lrpj

    Abstract

    Dark matter remains one of the most profound and unresolved mysteries in modern physics. To unravel its nature, numerous haloscope experiments have been implemented across various mass ranges. However, very few haloscope experiments have been conducted within the millimeter-wave frequency range, which is in the favored mass region for well-motivated dark matter candidates. Here we designed and constructed a millimeter-wave dielectric haloscope featuring a dark matter detector composed of dielectric disks and a mirror. Using this setup, we conducted a search for randomly polarized dark photon dark matter and found no evidence for its existence. Our results established new constraints on the kinetic mixing parameter in the mass range from 387.72 to 391.03  μeV, improving the existing limits by 2 orders of magnitude. With future enhancements, our system has the potential to explore new parameter space for dark photons as well as axion dark matter within the millimeter-wave frequency range.

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