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Search for "Invisible" Axion Dark Matter in the 3.3-4.2~{μ}eV Mass Range

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arxiv 2110.06096 v3 pith:OKWW7CV4 submitted 2021-10-12 hep-ex astro-ph.COphysics.ins-det

Search for "Invisible" Axion Dark Matter in the 3.3-4.2~{μ}eV Mass Range

ADMX Collaboration: C. Bartram , T. Braine , E. Burns , R. Cervantes , N. Crisosto , N. Du , H. Korandla , G. Leum
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P. Mohapatra T. Nitta L. J Rosenberg G. Rybka J. Yang John Clarke I. Siddiqi A. Agrawal A. V. Dixit M. H. Awida A. S. Chou M. Hollister S. Knirck A. Sonnenschein W. Wester J. R. Gleason A. T. Hipp S. Jois P. Sikivie N. S. Sullivan D. B. Tanner E. Lentz R. Khatiwada G. Carosi N. Robertson N. Woollett L. D. Duffy C. Boutan M. Jones B. H. LaRoque N. S. Oblath M. S. Taubman E. J. Daw M. G. Perry J. H. Buckley C. Gaikwad J. Hoffman K. W. Murch M. Goryachev B. T. McAllister A. Quiskamp C. Thomson M. E. Tobar
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We report the results from a haloscope search for axion dark matter in the $3.3\text{-}4.2~{\mu}$eV mass range. This search excludes the axion-photon coupling predicted by one of the benchmark models of "invisible" axion dark matter, the KSVZ model. This sensitivity is achieved using a large-volume cavity, a superconducting magnet, an ultra low noise Josephson parametric amplifier, and sub-Kelvin temperatures. The validity of our detection procedure is ensured by injecting and detecting blind synthetic axion signals.

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Cited by 4 Pith papers

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  1. Lights, Camera, Axion: Tracing Axions from Supernovae in the Diffuse $\gamma$-ray Sky

    hep-ph 2026-04 unverdicted novelty 7.0

    Axions produced in supernovae generate a diffuse gamma-ray signal through conversion in magnetic fields, yielding competitive constraints on the axion-photon coupling from COMPTEL, EGRET, and Fermi-LAT data plus forec...

  2. Landau-Zener formula and resonant axion conversion in neutron star magnetospheres

    hep-ph 2026-06 unverdicted novelty 6.0

    The Landau-Zener approximation for axion-photon conversion in neutron star magnetospheres fails when resonance width exceeds conversion region size, leading to revised axion constraints from optical-band searches.

  3. Audible Axion Magnetogenesis: Linking Intergalactic Magnetic Fields and Gravitational Waves

    hep-ph 2026-05 unverdicted novelty 5.0

    Axion-like particles in the trapped misalignment mechanism produce observable gravitational waves while generating intergalactic magnetic fields that exceed blazar lower bounds in the parameter space promising for gra...

  4. Serendipitous supersymmetric solution to the strong CP problem

    hep-ph 2026-07 conditional novelty 4.5

    Anomaly-free discrete R-symmetries plus Kim-Nilles regeneration of the mu term force an accidental U(1)_PQ whose spontaneous breaking yields a SUSY DFSZ axion that solves strong CP.