![Page 1: 2009 Florida Academy of Sciences at Saint Leo University, Saint Leo, Florida Performance comparison of the triple gas electron multiplier (GEM) and the](https://reader035.vdocuments.us/reader035/viewer/2022062806/5697bfd01a28abf838caac45/html5/thumbnails/1.jpg)
2009 Florida Academy of Sciences atSaint Leo University, Saint Leo, Florida
Performance comparison of the triple gas electron multiplier (GEM) and the drift tube muon detectors
used for muon tomography.
J. Locke, K. Gnanvo, R. Hoch, M. Hohlmann, D. Mitra.
Florida Institute of TechnologyDepartment of Physics and Space Sciences
150 West University BoulevardMelbourne, Florida 32901
![Page 2: 2009 Florida Academy of Sciences at Saint Leo University, Saint Leo, Florida Performance comparison of the triple gas electron multiplier (GEM) and the](https://reader035.vdocuments.us/reader035/viewer/2022062806/5697bfd01a28abf838caac45/html5/thumbnails/2.jpg)
Muon Tomography
![Page 3: 2009 Florida Academy of Sciences at Saint Leo University, Saint Leo, Florida Performance comparison of the triple gas electron multiplier (GEM) and the](https://reader035.vdocuments.us/reader035/viewer/2022062806/5697bfd01a28abf838caac45/html5/thumbnails/3.jpg)
Drift Tube vs. Gas Electron Multiplier (GEM) Detectors
![Page 4: 2009 Florida Academy of Sciences at Saint Leo University, Saint Leo, Florida Performance comparison of the triple gas electron multiplier (GEM) and the](https://reader035.vdocuments.us/reader035/viewer/2022062806/5697bfd01a28abf838caac45/html5/thumbnails/4.jpg)
Objective
Compare the performances of
drift tube and GEM
detectors used for
muon tomography.
![Page 5: 2009 Florida Academy of Sciences at Saint Leo University, Saint Leo, Florida Performance comparison of the triple gas electron multiplier (GEM) and the](https://reader035.vdocuments.us/reader035/viewer/2022062806/5697bfd01a28abf838caac45/html5/thumbnails/5.jpg)
Computer Simulation Tools• Geant4
– C++ based utility developed by the high energy physics community.
– Used to create geometry of scenarios and simulate particulate propagation through matter.
• CRY– Cosmic RaY muon production software. – Used to produce muons with momenta reflecting
observed natural momenta distributions .
• POCA– Point Of Closest Approach. – Used to calculate interaction points inside detectors,
where muons are likely to have scattered.
![Page 6: 2009 Florida Academy of Sciences at Saint Leo University, Saint Leo, Florida Performance comparison of the triple gas electron multiplier (GEM) and the](https://reader035.vdocuments.us/reader035/viewer/2022062806/5697bfd01a28abf838caac45/html5/thumbnails/6.jpg)
Scenario TestedBottom View Rear View
Targets (5) Engine
Detectors Targets (5)EngineBattery
Battery
Scenario exposed to cosmic ray muons for 10 minutes.
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Performance: Resolution
Drift Tubes
GEMs
Mean Scattering
Angle (degrees)
(mm)x(mm)y
(mm)z
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Performance: Distinguishing
Materials
U
Pb
Fe
Al W
Mean Scattering Angle(degrees)
Voxel
Drift Tubes
GEMs
U
Pb
Fe
Al W
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Performance: Muon
Coverage
Muons / Voxel
Max. Muon / Voxel
Drift Tubes
GEMs
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Conclusion
• GEM detectors are capable of higher resolution 3D reconstruction of scenarios than comparable drift tube detectors.
• GEM detectors are better capable of distinguishing between materials of similar densities than comparable drift tube detectors.
• GEM detectors are capable of higher coverage of muon activity within detector systems than comparable drift tube detectors.
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Future Objectives for Muon Tomography at Florida Tech
• Simulate different detector arrangements (i.e. a trapezoidal prism, instead of a box) to determine more efficient arrangements.
• Gather statistical data for scattering angles of different materials.
• Replace the POCA algorithm with EM or another more accurate reconstruction algorithm.
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2009 Florida Academy of Sciences atSaint Leo University, Saint Leo, Florida
Performance comparison of the triple gas electron multiplier (GEM) and the drift tube muon detectors
used for muon tomography.
J. Locke, K. Gnanvo, R. Hoch, M. Hohlmann, D. Mitra.
Florida Institute of TechnologyDepartment of Physics and Space Sciences
150 West University BoulevardMelbourne, Florida 32901