First Direct-Detection Constraints on eV-Scale Hidden-Photon Dark Matter with DAMIC at SNOLAB
arXiv:1611.03066 · doi:10.1103/PhysRevLett.118.141803
Abstract
We present direct detection constraints on the absorption of hidden-photon dark matter with particle masses in the range 1.2-30 eV with the DAMIC experiment at SNOLAB. Under the assumption that the local dark matter is entirely constituted of hidden photons, the sensitivity to the kinetic mixing parameter is competitive with constraints from solar emission, reaching a minimum value of 2.2 at 17 eV. These results are the most stringent direct detection constraints on hidden-photon dark matter in the galactic halo with masses 3-12 eV and the first demonstration of direct experimental sensitivity to ionization signals 12 eV from dark matter interactions.
arXiv comment5 pages, 5 figures
References in corpus (11)
- WISPy Cold Dark Matter
- Dark Light, Dark Matter and the Misalignment Mechanism
- Bosonic super-WIMPs as keV-scale dark matter
- New stellar constraints on dark photons
- Direct Detection Constraints on Dark Photon Dark Matter
- Solar constraints on hidden photons re-visited
- Massive hidden photons as lukewarm dark matter
- Absorption of light dark matter in semiconductors
- Search for low-mass WIMPs in a 0.6 kg day exposure of the DAMIC experiment at SNOLAB
- Experimental Search for Hidden Photon CDM in the eV mass range with a Dish Antenna
- Measurement of radioactive contamination in the high-resistivity silicon CCDs of the DAMIC experiment
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