Abstract
The UV-detectors of the CERES/NA45 experiment were originally conceived as parallel-plate counters with two-step amplification, an intermediate gate-electrode pair, and a final drift stage towards a pad electrode. Operated in beams of a few 106/burst protons or 32S-nuclei at 200 GeV/u, this scheme was found to suffer from excessive spark rates, even in the gated mode. The origin of the sparks is quantitatively explained by event-correlated slow secondary particles, creating avalanches above the critical threshold of ∼ 108 charges at the required gain of a few 105. This lack of sufficient dynamic range is also present in other schemes proposed in the literature; it severely limits the use of large-area parallel-plate counters for single-electron detection in a realistic high-energy physics environment. Possible improvements resulting from resistive anodes instead of metal meshes are also discussed. The spark problem of the CERES UV-detectors was solved by introducing wire amplification as the last stage. Laboratory tests showed a large increase in the dynamic range, due to a strong reduction (by factors of at least 20-30) of the net gain of the wire plane for high input charges via space-charge limitation. The residual spark rates of this scheme are lower by orders of magnitude and quite acceptable even for 32S-beams; gating was found to be unnecessary.
| Original language | English |
|---|---|
| Pages (from-to) | 231-240 |
| Number of pages | 10 |
| Journal | Nuclear Inst. and Methods in Physics Research, A |
| Volume | 343 |
| Issue number | 1 |
| DOIs | |
| State | Published - Apr 1 1994 |
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