Open AccessHelium Background in the D0 Detector Related to the Photomultiplier Tubes
Author(s) -
R. Rucinski
Publication year - 1998
Language(s) - English
Resource type - Reports
DOI - 10.2172/1032110
Subject(s) - helium , photomultiplier , helium ionization detector , liquid helium , nuclear physics , detector , cryogenics , dynode , physics , lambda point refrigerator , helium atom , materials science , atomic physics , optics , plasma , ion source , quantum mechanics
Helium is present in the earth's atmosphere at about 5 parts per million. (ref. Technology of liquid helium, NBS monograph 111). The D-Zero detector uses helium for the cryogenic cooling of its superconducting magnet and visible light photon counter (VLPC) electronics chips. In addition, the tevatron accelerator has superconducting magnets that use helium Due to the possibility of leaks or releases of helium from these helium lines and components, the background helium level in the collision hall may exceed the natural level of 5 ppm. This engineering note will quantify the probability and level of helium background in the D-Zero detector. The photomultiplier tubes used in the D-Zero detector are sensitive to an elevated helium atmosphere. This is due to the permeation rate of helium gas through the glass tube, into the vacuum space inside. It is very important for the helium atmosphere surrounding the photomultiplier tubes is known and controlled. If the level of helium in the vacuum tube reaches a level above 5 ppm, then the photomuliplier tube may no longer work as designed. The process is an irreversible one