Atomic Ionization by keV-scale Pseudoscalar Dark Matter Particles
arXiv:1002.2979 · doi:10.1103/PhysRevD.81.103520
Abstract
Using the relativistic Hartree-Fock approximation, we calculate the rates of atomic ionization by absorption of pseudoscalar particles in the mass range from 10 to 50 keV. We present numerical results for atoms relevant for the direct dark matter searches (e.g. Ar, Ge, I and Xe), as well as the analytical formula which fits numerical calculations with few per cent accuracy and may be used for multi-electron atoms, molecules and condensed matter systems.
4.5 pages, 3 figures
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- Dark matter scattering on electrons: Accurate calculations of atomic excitations and implications for the DAMA signal
- Constraints on dark photons and axion-like particles from SuperCDMS Soudan
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- Dark Matter Absorption via Electronic Excitations
- Millicharged Cosmic Rays and Low Recoil Detectors
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- New Atomic probes for Dark Matter detection: Axions, Axion-like particles and Topological Defects
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- Physical Signatures of Fermion-Coupled Axion Dark Matter
- New generation low-energy probes for ultralight axion and scalar dark matter
- Atomic ionization by scalar dark matter and solar scalars
- Migdal-type effect in the dark matter absorption process
- The Non-Relativistic Effective Field Theory Of Dark Matter-Electron Interactions
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