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Probing Dark Matter Axions using the Hyperfine Structure Splitting of Hydrogen Atoms

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arxiv 1912.11472 v5 pith:6KLNHC2V submitted 2019-12-24 hep-ph hep-exphysics.atm-clus

classification hep-phhep-exphysics.atm-clus
keywords axionshydrogendarkmatteratomicenergymassaxion-induced
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

QCD axions can be a substantial part of dark matter if their mass $m_a\sim10^{-5}$eV. Since the axions were created by the misalignment mechanism, their local energy spectrum density is large. Consequently, the axion-induced atomic transition rate is enhanced if the atomic energy gap matches the axion mass. The hyperfine splitting between the spin 0 singlet ground state and the spin 1 triplet state of hydrogen is $0.59\times10^{-5}$eV, which is close to the preferred mass of dark matter axions. With an energy gap adjustment by applying a weak Zeeman magnetic field, dark matter axions can induce atomic hydrogen transitions. Furthermore, because the total spins of the hydrogen triplet and singlet differ, the axion-induced transitions are detectable by a Stern--Gerlach apparatus or a sensitive magnetic field detector. A potential realization of the proposed scheme can be similar to existing hydrogen masers.

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  1. Dark matter pair absorption

    hep-ph 2025-07 conditional novelty 7.0 of 10

    Pair absorption of two dark matter particles in atomic transitions can probe electroweak-scale couplings of mu-eV-to-eV mass bosonic dark matter, and could bound the cosmic neutrino background overdensity near 10^9.

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