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Status and Perspectives on Axion Searches
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The search for axions and axion-like particles (ALPs) remains a major endeavor in modern physics investigation. Axions play essential roles in the quest to understand dark matter, the strong CP problem, and various astrophysical phenomena. This paper provides a very brief overview of the current status of experimental efforts, highlighting significant advancements, ongoing projects, and future opportunities. Particular attention is given to cavity haloscopes, helioscopes, and laboratory-based light-shining-through-wall experiments, as well as astrophysical probes. Some future perspectives are also discussed.
Forward citations
Cited by 8 Pith papers
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The Holographic QCD Axion in Five Dimensions
A 5D holographic QCD axion model identifies bulk modes for the axion and eta prime, traces the quality problem to insufficient compositeness, and finds the physical axion mostly in the bulk gauge field when quality is high.
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Solar axion searches with RES-NOVA: projected sensitivity and first prototype limit
RES-NOVA's projected 1 ton-year sensitivity reaches within a factor of ~2 of XENONnT on the solar-axion electron coupling, and a 32.4 g-day archaeological-lead prototype excludes new parts of the (g_ae, g_aγ) plane.
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Detection of Dark Matter Axions via the Quantum Hall Effect in a Resonant Cavity
A resonant cavity with a quantum Hall sample detects axion dark matter through photon absorption that produces a measurable ~5 mK temperature increase at millikelvin temperatures.
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Power of Axion Microwave Absorbed by Quantum Hall State in Haloscope
A QCD-axion haloscope using a GaAs quantum-Hall transition layer is estimated to absorb P_s ≈ 1.5×10^-23 W with SNR ≈ 2.3 after 100 s at T = 100 mK.
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Low-frequency radio telescopes sensitivity to light dark matter
The study calculates sensitivity of space- and Moon-based radio telescopes to resonant light dark matter conversion in solar system targets, finding encouraging prospects for dark photon searches with the Sun and axio...
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NuSTAR as an Axion Helioscope: probing axion-nucleon and axion-electron couplings
NuSTAR solar minimum data sets g_ae · g_aγ ≲ 1.1×10^{-24} GeV^{-1} and g_aN^eff · g_aγ ≲ 2.3×10^{-19} GeV^{-1} at 95% CL for m_a ≲ 10^{-6} eV.
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A Way of Axion Detection with Mass $10^{-4} \text{-}10^{-3}$eV Using Cylindrical Sample with Low Electric Conductivity
Proposes using low-conductivity cylindrical samples in strong B-fields to detect axion-induced bulk currents, with SNR estimates indicating feasibility for R=80 cm at 4 K.
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A Supersymmetric Extension of Axionic Electrodynamics: From Axions and Photons to Axinos and Photinos
Constructs supersymmetric axionic electrodynamics with axino-photino interactions, quartic couplings, and numerical bosonic solutions resembling magnetic vortices.
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