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Direct detection of sub-GeV dark matter

2011/08/31 by Rouven Essig, Jeremy Mardon, Tomer Volansky · 20 citations
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Dark matter #Particle Detector Development and Performance #Particle physics #Particle physics theoretical and experimental studies #Physics #astro-ph.CO #hep-ex #hep-ph

paper · pdf · doi:10.1103/physrevd.85.076007

published as Phys.Rev. D85 (2012) 076007 · 9 pages. Updated figure and references. Freeze-in region corrected. Other minor clarifications

arxiv created 2012/03/01 · openalex publication_date 2012/04/09 · arxiv updated 2012/06/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Direct detection strategies are proposed for dark matter particles with MeV to GeV mass. In this largely unexplored mass range, dark matter scattering with electrons can cause single-electron ionization signals, which are detectable with current technology. Ultraviolet photons, individual ions, and heat are interesting alternative signals. Focusing on ionization, we calculate the expected dark matter scattering rates and estimate the sensitivity of possible experiments. Backgrounds that may be relevant are discussed. Theoretically interesting models may be within reach using existing data and ongoing direct detection experiments. Significant improvements in sensitivity should be possible with dedicated experiments, opening up a window to new regions in dark matter parameter space.

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