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Etude de bruit de fond induit par les muons dans l'expérience ...

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tel-00724955, version 1 - 23 Aug 2012<br />

4 Muon <strong>de</strong>tection<br />

Contents<br />

4.1 Muon veto conventions<br />

4.2 Life time of the muon veto<br />

4.3 Muon rate<br />

4.4 Mean muon energy <strong>de</strong>posit per module<br />

4.5 Tracking muon candidates<br />

Who or<strong>de</strong>red that?<br />

I. I. Rabi.<br />

Muons are the only component of the primary cosmic ray interactions in the atmosphere<br />

that survives un<strong>de</strong>rground beyond the ∼ 10 mwe scale. And though<br />

there is a reduction of the cosmic muon flux by the rock overbur<strong>de</strong>n in LSM and<br />

equivalent laboratories of more than 106 com<strong>par</strong>ed to sea level, neutrons produced<br />

in <strong>de</strong>ep inelastic scattering (DIS) of cosmic <strong>muons</strong> are the most prominent background<br />

in the upcoming second generation experiments searching directly for Dark<br />

Matter. The i<strong>de</strong>ntification of <strong>muons</strong> in the vicinity of the Germanium <strong>de</strong>tectors allows<br />

a significant suppression of this background source and hence an improvement<br />

in the experimental sensitivity.<br />

The muon veto consists of 42 plastic scintillator modu<strong>les</strong>, read out at both ends<br />

with an electronics and a data read-out fully in<strong>de</strong>pen<strong>de</strong>nt from the bolometer system,<br />

except for a fiber connection transferring the overall experiment synchronization as<br />

well as some restricted information about muon hits, as <strong>de</strong>tailed in Section 3.3. The<br />

muon veto is the extreme outsi<strong>de</strong> layer of EDELWEISS-II, surrounding almost hermetically<br />

the experimental setup with a total surface of ∼ 100 m2 , see Figures 3.10<br />

and 3.11, page 69. The muon veto has been installed since May 2005 at the un<strong>de</strong>rground<br />

laboratory LSM in Modane, ready for data taking since September 2005 and<br />

stable in terms of long term measuring conditions since July 2006.<br />

4.1 Muon veto conventions<br />

The muon veto registers two kinds of data fi<strong>les</strong>: The scaler fi<strong>les</strong> ma<strong>de</strong> of raw data<br />

and the event data file.<br />

The raw data from the scaler cards correspond to any signal collected by the<br />

photomultipliers at the end of a si<strong>de</strong> of a module and above the threshold of the<br />

discriminator cards. It is the number of hits per channel per 15 min, with no other<br />

information. They are used to monitor the system, cf. Section 3.3.3. With a rate<br />

81<br />

4

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