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SENSEI: First Direct-Detection Constraints on Sub-GeV Dark Matter from a Surface Run
Michael Crisler1, Rouven Essig2, Juan Estrada1
1Fermi National Accelerator Laboratory, Post Office Box 500, Batavia, Illinois 60510, USA.
The Sub-Electron-Noise Skipper CCD Experimental Instrument (SENSEI) sets new dark matter detection limits using Skipper-CCD technology. This experiment searches for electron recoils, constraining sub-GeV dark matter particle interactions.
Area of Science:
- Particle physics
- Astrophysics
- Experimental physics
Background:
- Dark matter interactions with electrons are a key area of research.
- Skipper-CCD technology offers enhanced sensitivity for detecting low-energy events.
- Previous experiments have not focused on electron recoil detection for sub-GeV dark matter.
Purpose of the Study:
- To present the first results from a prototype Sub-Electron-Noise Skipper CCD Experimental Instrument (SENSEI).
- To search for sub-GeV dark matter particles interacting with electrons in silicon via electron recoils.
- To establish new direct-detection constraints for dark matter particle candidates.
Main Methods:
- Utilized a prototype SENSEI detector employing Skipper-CCD technology.
- Collected 0.019 gram-days of commissioning data above ground at Fermi National Accelerator Laboratory.
- Analyzed data for signals consistent with electron recoils from dark matter interactions.
Main Results:
- Established new direct-detection constraints for dark matter particles in the mass range of approximately 500 keV to 4 MeV.
- Disallowed previously allowed strongly interacting dark matter particles (masses ~500 keV to a few hundred MeV) due to surface data.
- Demonstrated the capability of Skipper-CCD technology for dark matter searches.
Conclusions:
- The SENSEI experiment successfully set new constraints on sub-GeV dark matter.
- The results highlight the potential of Skipper-CCD technology for future dark matter detection experiments.
- The findings have implications for various dark matter models, including those related to the EDGES anomaly.
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