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Transmon Qubit Constraints on Dark Matter-Nucleon Scattering

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arxiv 2405.00112 v2 pith:DF5WUYPL submitted 2024-04-30 hep-ph astro-ph.COhep-ex

classification hep-phastro-ph.COhep-ex
keywords darkmatterdevicesquasiparticletransmondensitiesenergymatter-nucleon
verification ladder T0 review T1 audit T2 compute T3 formal
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We recently pointed out that power measurements of single quasiparticle devices can be used to detect dark matter. These devices have the lowest known energy thresholds, far surpassing standard direct detection experiments, requiring energy deposition above only about an meV. We calculate dark matter induced quasiparticle densities in transmon qubits, and use the latest transmon qubit measurements that provide one of the strongest existing lab-based bounds on dark matter-nucleon scattering below about 100 MeV. We strongly constrain sub-component dark matter, using both a dark matter population thermalized in the Earth as well as the dark matter wind from the Galactic halo. We demonstrate future potential sensitivities using devices with low quasiparticle densities.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dark Matter Weather: Probing Sub-GeV Interactions with Earth-Shielding Modulation

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Daily Earth-shielding modulation of sub-GeV dark matter can separate dark-matter–electron from dark-matter–nucleon scattering, and the isoangle shape statistic provides a new validation handle for liquid-noble detectors.

  2. Complementary Planetary Spectroscopy Probes of Dark Matter

    hep-ph 2025-08 conditional novelty 6.0 of 10

    Dark matter annihilation energy deposited in planetary atmospheres and interiors, compared against existing UV airglow and heat flow measurements, yields new sub-GeV scattering constraints and long-lived mediator reach.

  3. Unconventional Materials for Light Dark Matter Detection

    hep-ph 2025-07 conditional novelty 6.0 of 10

    TiSe2, Sr2RuO4, and hole-doped diamond are projected to improve sub-MeV dark matter detection reaches by one to three orders of magnitude over existing proposals, with directional sensitivity from their anisotropic responses.

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