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The FEE Server Control Engine of the ALICE-TRD - Westfälische ...

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1 Introduction<br />

<strong>The</strong> standard model <strong>of</strong> elementary particles describes <strong>the</strong> particles we observe in <strong>the</strong><br />

universe and <strong>the</strong> ways <strong>the</strong>se particles interact. 1 According to <strong>the</strong> standard model<br />

all observed hadrons like protons or pions are composed <strong>of</strong> gluons and two or three<br />

quarks/anti-quarks. Quantum chromodynamics (QCD) describes <strong>the</strong> interactions between<br />

<strong>the</strong>se particles.<br />

In normal baryonic matter each quark, anti-quark or gluon is assigned to one hadron.<br />

Free (anti-)quarks or gluons have never been observed. This behavior is called confinement.<br />

Ano<strong>the</strong>r important property <strong>of</strong> <strong>the</strong> QCD is asymptotic freedom. At high energies,<br />

which is equivalent to small distances, <strong>the</strong> coupling strength between quarks and gluons<br />

becomes weak.<br />

In <strong>the</strong> very early universe, up to about 10 µs after <strong>the</strong> Big Bang <strong>the</strong> temperature was<br />

above a critical temperature Tc = 150 − 190 MeV [BMS07]. At <strong>the</strong>se temperatures quarks<br />

and gluons are not confined to hadrons but can move freely. This state is called a quarkgluon<br />

plasma (QGP). When <strong>the</strong> universe expanded, it cooled down and <strong>the</strong> quarks and<br />

gluons were confined inside hadrons. In <strong>the</strong> present-day universe a QGP may only exist<br />

inside <strong>of</strong> neutron stars if <strong>the</strong> densities are high enough.<br />

In a laboratory <strong>the</strong> QGP can be created by colliding two nuclei at ultra-relativistic<br />

center-<strong>of</strong>-mass energies. For a short time <strong>the</strong> energy density in <strong>the</strong> collision zone is high<br />

enough to create a QGP. Measuring <strong>the</strong> properties <strong>of</strong> <strong>the</strong> QGP and investigating <strong>the</strong> phase<br />

transition from a QGP to normal baryonic matter is very important. Such measurements<br />

can be used to check QCD calculations and <strong>the</strong>y increase our knowledge about <strong>the</strong> history<br />

<strong>of</strong> <strong>the</strong> universe. <strong>The</strong> Super Proton Synchrotron (SPS) at CERN was <strong>the</strong> first accelerator<br />

which saw hints for <strong>the</strong> creation <strong>of</strong> a QGP [CER00]. In 2009 <strong>the</strong> new Large Hadron Collider<br />

(LHC) at CERN near Geneva will start its regular operation. It is capable to collide<br />

heavy ions at center-<strong>of</strong>-mass energies up to √ sNN = 5.5 TeV which is about 30 times<br />

more <strong>the</strong>n RHIC 2 energies [BMS07]. However, most <strong>of</strong> <strong>the</strong> time <strong>the</strong> LHC will run protonproton<br />

collisions mainly to look for <strong>the</strong> Higgs boson which is <strong>the</strong> last undetected particle<br />

<strong>of</strong> <strong>the</strong> standard model and search for physics beyond <strong>the</strong> standard model. <strong>ALICE</strong> as one<br />

<strong>of</strong> <strong>the</strong> four experiments at LHC is <strong>the</strong> only dedicated heavy ion experiment.<br />

In this diploma <strong>the</strong>sis <strong>the</strong> control engine for <strong>the</strong> transition radiation detector (<strong>TRD</strong>) <strong>of</strong><br />

<strong>ALICE</strong> has been redesigned, implemented and tested. Based on this s<strong>of</strong>tware a procedure<br />

was developed to check proper cooling <strong>of</strong> <strong>the</strong> front end electronics <strong>of</strong> <strong>the</strong> <strong>TRD</strong>.<br />

1 Nowadays it is known that <strong>the</strong> standard model cannot be complete because it fails describing some important<br />

observations like <strong>the</strong> nature <strong>of</strong> dark matter.<br />

2 <strong>The</strong> Relativistic Heavy Ion Collider (RHIC) located at <strong>the</strong> Brookhaven National Laboratory at Long Island<br />

(USA) was <strong>the</strong> most powerful heavy ion collider before LHC was build<br />

7

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