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Supersymmetry or Universal Extra Dimensions? Utilizing the ATLAS Experiment at CERN
Supersymmetry and Universal Extra Dimensions are just two of an array of popular and enticing extensions to the Standard Model. The work presented in this thesis evaluates the feasibility of differentiating between these two models by measuring the spins of the new particles, utilising the ATLAS exp...
Autor principal: | |
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Lenguaje: | eng |
Publicado: |
2009
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/2318214 |
Sumario: | Supersymmetry and Universal Extra Dimensions are just two of an array of
popular and enticing extensions to the Standard Model. The work presented in
this thesis evaluates the feasibility of differentiating between these two models
by measuring the spins of the new particles, utilising the ATLAS experiment at
the Large Hadron Collider at CERN. The method presented depends upon the
use of an angular variable, cos θ∗
ll, which is sensitive to the polar angle in the
direct slepton pair production process: qq → Z0/γ∗ → ˜l± ˜l∓ → χ˜0
1l
±χ˜0
1l
∓. This
angular variable is advantageous since it is longitudinally boost invariant along
the beam axis. This allows it to be used at the Large Hadron Collider where the
initial centre-of-mass frame of reference is unknown and unrecoverable owing to
the presence of invisible particles in the event. The work invoked Monte Carlo
events, fully simulated in accordance with the mSUGRA Supersymmetry model
corresponding to a selected production point in mSUGRA space of the ATLAS
detector. It was demonstrated that, using this method and given the Monte
Carlo simulation at this test point, the Large Hadron Collider can distinguish
between the supersymmetric production angular distribution and that of UED
using 30 fb−1 of integrated luminosity. A further part of the work involved an
investigation into part of the innermost detector system of ATLAS. The work
investigated the operational performance of a certain fraction of semiconductor
tracker barrel modules utilizing data acquired during cosmic commissioning tests
carried out at CERN in 2006. This included measuring the noise occupancy levels
and subsequently identifying any problematic modules in the process. Eight problematic modules were identified, forming three distinct classes, each class
pointing toward a different type of problem. Furthermore, an anomaly, the socalled
zeroth time bin anomaly, was found and prompted further investigation to
its root cause. |
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