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Sub-MeV Dark Matter Detection with Bilayer Graphene

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arxiv 2312.00866 v2 pith:MSV4RQNQ submitted 2023-12-01 hep-ph astro-ph.COcond-mat.mes-hall

classification hep-phastro-ph.COcond-mat.mes-hall
keywords darkmatterbilayerdetectorexperimentgraphenedetectionmass
verification ladder T0 review T1 audit T2 compute T3 formal
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The light dark matter mass regime has emerged as the next frontier in the direct detection experiment due to the lack of any detection signal in the higher mass range. In this paper, we propose a new detector material, a bilayer stack of graphene to detect sub-MeV dark matter. Its voltage-tunable low energy sub-eV electronic band gap makes it an excellent choice for the detector material of a light dark matter search experiment. We compute its dielectric function using the random phase approximation and estimate the projected sensitivity for sub-MeV dark matter-electron scattering and sub-eV dark matter absorption. We show that a bilayer graphene dark matter detector can have competitive sensitivity as other candidate target materials, like a superconductor, but with a tunable threshold energy in this mass regime. The dark matter scattering rate in bilayer graphene is also characterized by a daily modulation from the rotation of the Earth which may help us mitigate the backgrounds in a future experiment. We also outline a detector design concept and provide noise estimates that can be followed to setup an experiment in future.

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Forward citations

Cited by 3 Pith papers

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

  1. 1D Luttinger Modes in Carbon Nanotubes as keV Dark Matter Detector

    hep-ph 2026-07 conditional novelty 8.0 of 10

    Metallic carbon nanotube plasmon modes can serve as a new target for sub-MeV dark matter detection, with projected sensitivity reaching the keV–MeV freeze-in benchmark.

  2. First-principles upper bounds on dark matter-electron scattering rates from condensed matter sum rules

    hep-ph 2026-08 conditional novelty 6.0 of 10

    Dark matter-electron scattering rates in isotropic materials are bounded from above by a universal expression depending only on plasma frequency, mass density, and static dielectric function.

  3. Indirect dark matter searches with neutrino telescopes via energetic cosmic showers

    hep-ph 2025-09 reject novelty 3.0 of 10

    Bounds on Z'-mediated dark matter are derived from neutrino telescopes, freeze-in, and cosmic strings, but the telescope bounds rest on comparing a Galactic-center flux to faraway sources.

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