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Direct dark matter search with the CRESST-III experiment - status and perspectives
- Publication Year :
- 2017
-
Abstract
- The CRESST-III experiment, located in the Gran Sasso underground laboratory (LNGS, Italy), aims at the direct detection of dark matter (DM) particles. Scintillating CaWO(4) crystals operated as cryogenic detectors are used as target material for DM-nucleus scattering. The simultaneous measurement of the phonon signal from the CaWO(4) crystal and of the emitted scintillation light in a separate cryogenic light detector is used to discriminate backgrounds from a possible dark matter signal. The experiment aims to significantly improve the sensitivity for low-mass (≲ 5-10 GeV/c(2)) DM particles by using optimized detector modules with a nuclear recoil-energy threshold ≲ 100 eV. The current status of the experiment as well as projections of the sensitivity for spin-independent DM-nucleon scattering will be presented.
- Subjects :
- Physics
History
Scintillation
Physics::Instrumentation and Detectors
Scattering
Dark matter
Detector
Astrophysics::Instrumentation and Methods for Astrophysics
Elementary particle
Cryogenics
010402 general chemistry
01 natural sciences
0104 chemical sciences
Computer Science Applications
Education
Baryon
Nuclear physics
0103 physical sciences
Scintillation counter
High Energy Physics::Experiment
Nuclear Experiment
010303 astronomy & astrophysics
Dark matter: direct detection | detector: cryogenics | sensitivity | Gran Sasso | scattering | crystal | scintillation counter | background | nucleus | phonon | CRESST
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....7f742453cd5d05f616f0a484e7c8005e