Nuclear Tracks from Cold Dark Matter Interactions in Mineral Crystals: A Computational Study
arXiv:astro-ph/9505055 · doi:10.1016/0168-583X(94)00543-5
Abstract
Recoiling nuclei from Cold Dark Matter (CDM) elastic scattering interactions with the constituent elements of some minerals may produce etchable damage tracks in the crystal structure. Present calculations show that in muscovite mica, CDM tracks from recoiling potassium atoms could be readily distinguished from others due to alpha-decays in the uranium and thorium chains. Under favorable conditions, this technique could greatly improve the existing limits on Weakly Interacting Massive Particles as the constituents of the galactic halo.
PostScript, 15 pages, 3 figures
References in corpus (1)
Cited by in corpus (14)
- Paleo-detectors: Searching for Dark Matter with Ancient Minerals
- Searching for Dark Matter with Paleo-Detectors
- Ultra-Heavy Dark Matter Search with Electron Microscopy of Geological Quartz
- Digging for Dark Matter: Spectral Analysis and Discovery Potential of Paleo-Detectors
- Paleo-Detectors for Galactic Supernova Neutrinos
- Mineral Detection of Neutrinos and Dark Matter. A Whitepaper
- Directional Detection of Dark Matter Using Solid-State Quantum Sensing
- Measuring Changes in the Atmospheric Neutrino Rate Over Gigayear Timescales
- Comments on "Limits on Dark Matter Using Ancient Mica"
- New Projections for Dark Matter Searches with Paleo-Detectors
- Constraints on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes
- Clumpy Cold Dark Matter and Biological Extinctions
- Particle detection and tracking with DNA
- Galactic Geology: Probing Time-Varying Dark Matter Signals with Paleo-Detectors