Direct Detection of Sub-GeV Dark Matter
arXiv:1108.5383 · doi:10.1103/PhysRevD.85.076007
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 can be probed with existing technologies, and may even be within reach using 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.
9 pages. Updated figure and references. Freeze-in region corrected. Other minor clarifications
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- Mapping the evolution of supernova-neutrino-boosted dark matter within the Milky Way
- Naturally Resonant Dark Matter from Extra Dimensions
- Thermal Leptophilic Light Vector Dark Matter with Spinor Mediator and Muon (g-2) Anomaly
- New constraints on dark matter from superconducting nanowires
- On the dark matter origin of an LDMX signal
- Dark Matter Detection With Bound Nuclear Targets: The Poisson Phonon Tail
- Solar Reflected Dark Matter under the Influence of a Dark Magnetic Field
- Production of Dark Photons through Higher Electromagnetic Moments at LDMX: Simulations and Model Discrimination
- Constraining light dark matter in vector-scalar portals with COSI and AMEGO-X
- First direct search for light dark matter interactions in a transition-edge sensor
- Study of sub-GeV Dipolar Dark States at SND@LHC within Invisible Bounds on Meson Decays
- Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection
- Scattering meets absorption in dark matter detection
- Direct Detection and Cosmological Constraints of Dark Matter with Dark Dipoles
- Hydrogenated carbon structures as directional sub-GeV dark matter detectors
- Constraining the heavy leptophilic neutral gauge bosons through the , , and decays