Projected Sensitivity of DMRadio-m$^3$: A Search for the QCD Axion Below $1\,\mu$eV

DMRadio Collaboration, L. Brouwer, S. Chaudhuri, H. -M. Cho, J. Corbin, W. Craddock, C. S. Dawson, A. Droster,J. W. Foster,J. T. Fry, P. W. Graham,R. Henning,K. D. Irwin, F. Kadribasic, Y. Kahn,A. Keller, R. Kolevatov, S. Kuenstner, A. F. Leder, D. Li,J. L. Ouellet, K. Pappas,A. Phipps, N. M. Rapidis, B. R. Safdi, C. P. Salemi, M. Simanovskaia, J. Singh,E. C. van Assendelft,K. van Bibber, K. Wells,L. Winslow, W. J. Wisniewski,B. A. Young

arxiv(2022)

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摘要
The QCD axion is one of the most compelling candidates to explain the dark matter abundance of the universe. With its extremely small mass ($\ll 1\,\mathrm{eV}/c^2$), axion dark matter interacts as a classical field rather than a particle. Its coupling to photons leads to a modification of Maxwell's equations that can be measured with extremely sensitive readout circuits. DMRadio-m$^3$ is a next-generation search for axion dark matter below $1\,\mu$eV using a $>4$ T static magnetic field, a coaxial inductive pickup, a tunable LC resonator, and a DC-SQUID readout. It is designed to search for QCD axion dark matter over the range $20\,\mathrm{neV}\lesssim m_ac^2\lesssim 800\,\mathrm{neV}$ ($5\,\mathrm{MHz}<\nu<200\,\mathrm{MHz}$). The primary science goal aims to achieve DFSZ sensitivity above $m_ac^2\approx 120$ neV (30 MHz), with a secondary science goal of probing KSVZ axions down to $m_ac^2\approx40\,\mathrm{neV}$ (10 MHz).
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