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  • Letter
  • Open Access

Hydrogenated carbon structures as directional sub-GeV dark matter detectors

Tomás Arias1, Antonino Bellinvia2, Gianluca Cavoto2,3,*, Angelo Esposito2,3,†, Francesco Pandolfi3,‡, Guglielmo Papiri1,§, Antonio D. Polosa2,3,∥, and Tyler Wu1

  • *Contact author: gianluca.cavoto@roma1.infn.it
  • †Contact author: angelo.esposito@uniroma1.it
  • ‡Contact author: francesco.pandolfi@roma1.infn.it
  • §Contact author: gp343@cornell.edu
  • ∥Contact author: antonio.polosa@roma1.infn.it

Phys. Rev. D 114, L011702 – Published 13 July, 2026

DOI: https://doi.org/10.1103/ym4j-8zlp

Abstract

We propose hydrogenated carbon structures as targets with a remarkable sensitivity to dark matter–nucleon interactions, in the mass range between 1 MeV and 100 MeV. The ejection of a proton following the interaction with a dark matter particle is a quasielastic process, with an extremely small energy threshold and a clear experimental signature. The proposed detectors are simple, technologically ready, and inexpensive. Yet, they can be considerably more sensitive than current experiments. They also allow strong directionality to be used toward efficient background rejection.

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