Progress in Ge detector technology has resulted in ultralow backgrounds of less than 0.3 counts keV−1 kg−1 d−1 at energies between 5 and 12 keV, and less than 1.0 counts kev−1 kg−1 d−1 for energies between 3 and 5 keV. Coupled with good energy resolution, 0.4 keV FWHM at 10 keV, this allows searches for DM particles with m ≥8 GeV/c2.
Electromagnetic interference and acoustical pick-up are the main sources of background in the best Ge detectors. These problems are even more important in cryogenic WIMP detectors under development. A PC-based on line pulse shape analysis system is presented which permits rejection of about 95% percent of the EMI/ acoustical background. The hardware uses a low cost, commercially available digital storage oscilloscope. The software consists of about 20,000 lines of code in Pascal and assembly language. We tested this system using a low radioactive background Ge-system on the Earth's surface. For low energy events (27 keV photons) this system permits improvement in the background from 0.1 cpm to 2 cpd.
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Sagdeev, I.R., Drukier, A.K. & Welsh, D.J. Data acquisition system for dark matter detectors. J Low Temp Phys 93, 761–766 (1993). https://doi.org/10.1007/BF00693509
- Dark Matter
- Assembly Language
- Storage Oscilloscope
- Matter Detector
- Digital Storage Oscilloscope