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development of micro-pattern gaseous detectors – gem - LMU

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2<br />

Figure 2: Schematics <strong>of</strong> the whole ATLAS detector [ATLA 10].<br />

field <strong>of</strong> 2 T. The hadronic (“Tile Calorimeter”) and electromagnetic (“Liquid Argon”) calorimeters<br />

are responsible for measuring the energy deposited by the corresponding particle in the material.<br />

In the outer region the muon chambers surround the detector in three layers. Only muons reach<br />

this area as all other particle are supposed to be absorbed in the inner layers. The muon system<br />

consists <strong>of</strong> cathode strip chambers (CSC) and Ar/CO2 filled drift tube chambers placed in a toroidal<br />

magnetic field <strong>of</strong> 0.4 T for measuring the momentum <strong>of</strong> the traversing charged muons by their radius<br />

<strong>of</strong> curvature. Resistive plate chambers and thin gap chambers provide the trigger.<br />

Figure 3: Expected background rates in Hz<br />

cm2 <br />

at five times LHC luminosity [Loeb 10].<br />

Additionally to the primary collision products from the proton-proton collision, background radiation<br />

is produced, mostly by interactions in the collimator. For the planned luminosity upgrade to<br />

5 · 10 34 cm −2 s −1 for SuperLHC the proportionally increased background rate will decrease the performance<br />

<strong>of</strong> specific detector regions.<br />

Fig. 3 shows the expected background rate in the muon spectrometer. Mostly affected are the CSC<br />

and the muon chambers sitting close by. Estimated background rates in the detector reach here values<br />

<strong>of</strong> 8500Hz/cm 2 . Due to their intrinsic insensitivity to space charge effects, large area GEM <strong>detectors</strong><br />

are considered as replacement candidates.<br />

To study the influence <strong>of</strong> high radiation background on ATLAS MDT chambers our working group

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