The existence of a significant non-baryonic component to the Universe is widely accepted, with worldwide efforts underway trying to detect this so-called dark matter. The ZEPLIN-III detector utilises liquid xenon (Xe) as a target medium in the search for the expected rare interactions of Weakly Interacting Massive Particles, or WIMPs, with ordinary baryonic matter. The neutralino, arising in supersymmetric extensions to the standard model of particle physics, provides a particularly well-motivated candidate. The ZEPLIN-III experiment, operating in two-phase (liquid/gas) mode, measures both the scintillation and ionisation signatures produced during an interaction. The first science run (FSR) of ZEPLIN-III was performed during three months in 2008. The run culminated in a published result which excluded a WIMP-nucleon interaction cross-section above 8:1 x 10-8 pb for a 60 GeVc-2 WIMP at the 90% confidence level. ZEPLIN-III then entered an upgrade period where the photomultiplier tube (PMT) array, previously the dominant source of background, was replaced with new, ultra-low background, PMTs. The radio-contamination of components used to make these PMTs has been thoroughly studied and their impact on the background rates in ZEPLIN-III characterised. Additionally, a new 1.5 tonne plastic scintillator veto detector was constructed, increasing the ability to reject WIMPlike signals caused by neutron induced nuclear recoil events and improving the γ-ray discrimination capability of ZEPLIN-III. The second science run (SSR) of ZEPLIN-III began in June 2010 and continued for 6 months, with a projected upper limit for the interaction cross-section of 1:52 x 10-8 pb for a 55 GeVc-2 WIMP at the 90% confidence level.

L’imagerie 3γ est une nouvelle technique d’imagerie médicale nucléaire qui a été proposée au laboratoire Subatech. Cette technique consiste à localiser tridimensionellement la position de la désintégration d’un radioisotope innovant émetteur (β+, γ), le 44Sc. Il s’agit pour cela d’associer la détection des deux photons gamma de 511 keV issus de la désintégration d’un positon, assurée par une couronne de détecteurs de tomogaphie à émission de positon, à la détection dutroisième photon par un télescope Compton au xénon liquide. La position de l’interaction entre le photon et le xénon, ainsi que l’énergie déposée, sont relevées grâce à la mesure du signal d’ionisation à l’aide d’un chambre MICROMEGAS (MICROMEsh GAseousStructure), tandis que le déclenchement de l’acquisition et la mesure du temps de l’interaction sont assurés parla détection du signal de scintillation. Le principe de la TPC est ainsi utilisé pour l’imagerie Compton.Afin de faire la preuve expérimentale de faisabilité de l’imagerie 3γ, un prototype de petite dimension, XEMIS (XEnon Medical Imaging System), a été développé.Cette thèse constitue une étape importante vers cette preuve de faisabilité. Les travaux qui y sont exposés portent sur la caractérisation de la réponse du détecteur pour un faisceau de gammas de 511 keV et sur l’analyse des données qui en sont issues. La mesure des résolutions en énergie et temporelle seront exposés, ainsi que celle de la pureté du xénon liquide. / 3γ imaging is a new nuclear medical imaging technique which has been suggested by Subatech laboratory. This technique involves locating three-dimensional position of the decay of an innovative radioisotope (β+, γ) emitter the 44Sc. The principle consist in the detection of two photons of 511 keV gamma rays from the decay of the positron, provided by a PET ring detector, associated to the detection of the third photon by a Liquid xenon Compton telescope. The energy deposited in the interaction between the photon and xenon and its position are identified by measuring the ionization signal with a MICROMEGAS chamber (MicroMesh Gaseous Structure), while the trigger and time measurement of the interaction are provided by the detection of thescintillation signal. The principle of the TPC is thus usedto Compton imaging.In order to demonstrate experimentally the feasibility of imaging 3γ, a small prototype, XEMIS (Xenon MedicalImaging System) was developed. This thesis is an important step towards the proof of feasibility. In this work are exposed the characterization of the detector response for a beam of 511 keV gamma rays and the analysis of data derived from it. The measurement of energy and time resolutions will be presented, as well as the purity of the liquid xenon.

The prospects for enhanced Positron Emission Tomography imaging using liquid xenon (LXe) gamma ray detectors had been examined. Monte-Carlo simulations using GEANT4 were performed and the results were used to study the expected performance of a small animal PET scanner in comparison with a simulated conventional small animal scanner (LSO Focus 120). A NEMA-like cylinder phantom and an image contrast phantom were simulated with both scanners to compare performance characteristics. A Compton reconstruction algorithm was developed for the LXe scanner, and its performance and limitations studied.

The prospects for enhanced Positron Emission Tomography imaging using liquid xenon (LXe) gamma ray detectors had been examined. Monte-Carlo simulations using GEANT4 were performed and the results were used to study the expected performance of a small animal PET scanner in comparison with a simulated conventional small animal scanner (LSO Focus 120). A NEMA-like cylinder phantom and an image contrast phantom were simulated with both scanners to compare performance characteristics. A Compton reconstruction algorithm was developed for the LXe scanner, and its performance and limitations studied.

The prospects for enhanced Positron Emission Tomography imaging using liquid xenon (LXe) gamma ray detectors had been examined. Monte-Carlo simulations using GEANT4 were performed and the results were used to study the expected performance of a small animal PET scanner in comparison with a simulated conventional small animal scanner (LSO Focus 120). A NEMA-like cylinder phantom and an image contrast phantom were simulated with both scanners to compare performance characteristics. A Compton reconstruction algorithm was developed for the LXe scanner, and its performance and limitations studied. / Science, Faculty of / Physics and Astronomy, Department of / Graduate

An overwhelming majority of matter in the Universe is dark matter, a substance unlike anything we know. Detecting dark matter particles requires ruling out observed phenomena caused by known particles. This thesis advances efforts toward the detection of dark matter using one of the most sensitive particle detection technologies: the dual-phase liquid xenon time projection chamber. Specifically, data from the XENON1T Experiment, located in Italy, and the Purdue small-scale ASTERiX detector are analyzed. A background of Lead-214 beta decay events can be mitigated by tracing the radioactive Radon-222 decay chain in XENON1T. However, a preliminary reduction of background has a high cost to exposure. Research on several topics was conducted with Purdue undergraduates, including a search for dark matter particles up to the Planck Mass, characterizing backgrounds due to muons, and searching for Boron-8 solar neutrino signals. XENON1T single-scatter dark matter limits were extended to a particle mass of 10¹⁸GeV/c². The ASTERiX detector was modified to characterize a significant background to the smallest detectable energy signatures: single- and few-electron ionization signals. Infrared light was determined to be ineffective at reducing this background, and their rates were observed to decrease inversely with time since an energetic interaction according to a power law. The rates of single- and few- electron backgrounds increase linearly with increased applied extraction fields and increased depth of the initial interaction in the detector. These results indicate that these backgrounds originate at the liquid-gas interface of dual-phase detectors. In exploring a single-photon threshold for initial scintillation signals, a previously unconsidered background of large dark count signals in the photosensors became apparent. The high background of small ionization signals and large dark count signals deterred a search for Boron-8 solar neutrino interactions in XENON1T. These studies are vital to mitigating backgrounds and improving the sensitivity of liquid xenon time projection chambers to new physical phenomena.

Astrophysical observations give convincing evidence for a vast non-baryonic component, the so-called dark matter, accounting for over 20% of the overall content of our Universe. Direct dark matter search experiments explore the possibility of interactions of these dark matter particles with ordinary baryonic matter via elastic scattering resulting in single nuclear recoils. The ZEPLIN-III detector operated on the basis of a dualphase (liquid/gas) xenon target, recording events in two separate response channels { scintillation and ionisation. These allow discrimination between electron recoils (from background radiation) and the signal expected from Weakly Interacting Massive Particle (WIMP) elastic scatters. Following a productive first exposure, the detector was upgraded with a new array of ultra-low background photomultiplier tubes, reducing the electron recoil background by over an order of magnitude. A second major upgrade to the detector was the incorporation of a tonne-scale active veto detector system, surrounding the WIMP target. Calibration and science data taken in coincidence with ZEPLIN-III showed rejection of up to 30% of the dominant electron recoil background and over 60% of neutron induced nuclear recoils. Data taking for the second science run finished in May 2011 with a total accrued raw fiducial exposure of 1,344 kg days. With this extensive data set, from over 300 days of run time, a limit on the spin-independent WIMP-nucleon cross-section of 4.8 10-8 pb near 50 GeV/c2 WIMP mass with 90% confidence was set. This result combined with the first science run of ZEPLIN-III excludes the scalar cross-section above 3.9 10-8 pb. Studying the background data taken by the veto detector allowed a calculation of the neutron yield induced by high energy cosmic-ray muons in lead of (5.8 0.2) 10-3 neutrons/muon/(g/cm2) for a mean muon energy of 260 GeV. Measurements of this kind are of great importance for large scale direct dark matter search experiments and future rare event searches in general. Finally, this work includes a comprehensive measurement of the energy dependent quenching factor for low energy nuclear recoils in a plastic scintillator, such as from the ZEPLIN-III veto detector, increasing accuracy for future simulation packages featuring large scale plastic scintillator detector systems.

Les travaux décrits dans cette thèse sont centrés sur la caractérisation et l’optimisation d’une camera Compton à phase unique au xénon liquide pour des applications médicales. Le détecteur a été conçu pour exploiter les avantages d’une technique d’imagerie médicale innovante appelée l’imagerie 3γ. Elle vise à l’obtention de la position en 3D d’une source radioactive avec une très haute sensibilité et une réduction importante de la dose administrée au patient. L’imagerie 3γ est basée sur la détection en coïncidence de 3 photons gamma émis par un émetteur spécifique (+β, γ), le 44Sc. Un premier prototype de camera Compton au xénon liquide a été développé par le laboratoire Subatech à travers le projet XEMIS (Xenon Medical Imaging System), pour démontrer la faisabilité de l’imagerie 3γ. Ce nouveau système de détection comporte un système de cryogénie avancé et une électronique front-end à très faible bruit qui fonctionne à la température du xénon liquide. Ce travail a contribué à la caractérisation de la réponse du détecteur et à l’optimisation de la mesure du signal d’ionisation. L'influence de la grille de Frisch sur le signal mesuré a été particulièrement étudiée. Les premières preuves de la reconstruction Compton en utilisant une source de ²²Na (β+, Eγ = 1.274 MeV) sont aussi rapportées dans cette thèse et valident la preuve de concept de la faisabilité de l’imagerie 3γ. Les résultats présentés dans cette thèse ont joué un rôle essentiel dans le développement d’une camera Compton au xénon liquide de grandes dimensions pour l’imagerie des petits animaux. Ce nouveau détecteur, appelée XEMIS2, est maintenant en phase de construction. / The work described in this thesis is focused on the characterization and optimization of a single-phaseliquid xenon Compton camera for medical imaging applications. The detector has been conceived to exploit the advantages of an innovative medical imaging technique called 3γ imaging, which aims to obtain aprecise 3D location of a radioactive source with high sensitivity and an important reduction of the dose administered to the patient. The 3γ imaging technique is based on the detection in coincidence of 3gamma rays emitted by a specific (+β, γ) emitter radionuclide,the 44Sc. A first prototype of a liquid xenon Compton camera has been developed by Subatech laboratory within the XEMIS (Xenon Medical Imaging System) project, to proof the feasibility of the 3γ imaging technique. This new detection framework is based on an advanced cryogenic system and an ultra-low noise front-end electronics operating at liquid xenon temperature. This work has contributed to the characterization of the detector response and the optimization of the ionization signal extraction. A particular interest has been given to the influence of the Frisch grid on the measured signals. First experimental evidences of the Compton cone reconstruction using asource of ²²Na (β+, Eγ = 1.274 MeV) are also reported in this thesis, which demonstrate the proof of concept of the feasibility of the 3γ imaging. The results reported in this thesis have been essential for the development of a larger scale liquid xenon Compton camera for small animal imaging. This new detector, called XEMIS2, is now in phase of construction.

L’imagerie 3γ est une technique innovante d’imagerie médicale nucléaire qui est étudiée au laboratoire SUBATECH. Elle repose sur la localisation tridimensionnelle d’un radioisotope émetteur (β+, γ), le 44Sc, à l’aide d’un télescope Compton au xénon liquide. Le lieu de désintégration de ce radioisotope est obtenu par l’intersection de la ligne de réponse, construite à partir de la détection des deux photons de 511 keV issus de l’annihilation d’un positron, et du cône déterminé à partir du troisième photon. Un prototype de petite dimension XEMIS1 (XEnon Medical Imaging System) a été développé afin de faire la preuve expérimentale de la faisabilité de l’imagerie à 3γ. Les résultats de ce prototype sont très promoteurs en terme de résolution en énergie, de pureté du xénon liquide et de faible bruit électronique. La simulation Monte Carlo est un outil indispensable pour accompagner la R&D et évaluer les performances de la nouvelle technique d’imagerie proposée. Les travaux rapportés dans cette thèse concernent le développement de la simulation du système d’imagerie 3γ avec GATE (Geant4 Application for Tomographic Emission). De nouvelles fonctionnalités ont été implémentées dans GATE afin de simuler un détecteur de type TPC (Time Projection Chamber). Nous avons effectué une simulation du prototype XEMIS1 et obtenu des résultats en bon accord avec nos données expérimentales. La prochaine étape du projet consiste à construire une caméra cylindrique au xénon liquide pour l’imagerie du petit animal. Les résultats des simulations de cette caméra présentés dans cette thèse montrent la possibilité de localiser chaque désintégration le long de la ligne de réponse avec une très bonne précision et une bonne sensibilité de détection. Des premières images de fantômes simples, réalisées évènements par événements, et après reconstruction tomographiques ont également présentées. / Nuclear medical 3γ imaging is an innovative technique which is studied at the SUBATECH laboratory. It isbased on the three-dimensional localization of a (β+, γ) radioisotope emitter, the 44Sc, by using a liquid xenon Compton telescope. The position of the disintegration of this radioisotope is obtained by the intersection of the line of response, built by the detection of two 511 keVphotons from the annihilation of a positron, and the cone determined by the third photon. A small prototype XEMIS1 (XEnon Medical Imaging System) was developed to demonstrate experimentally the feasibility of 3γ imaging. The results of this prototype are quite encouraging in terms of energy resolution, purity of liquid xenon and electronic noise. The Monte Carlo simulation is an indispensable tool to support the R&D and to evaluate the new proposed technique of imaging ; this thesis work is to develop the simulation of 3γ imaging system by using GATE (Geant4 Application for Tomographic Emission). New functionalities have been added to GATE to simulate a TPC (Time Projection Chamber) detector. We performed a simulation of XEMIS1 prototype and obtained results in good agreement with our experimental data. The next step of the project is to build a full liquid xenon cylindrical camera for the small animal imaging. The results presented in this thesis of the simulations of this camera demonstrate the ability to locate every decayalong the line of response with very good accuracy and good detection sensitivity. The first direct images of simple phantoms, realized event by event, and after tomographic reconstruction are also presented.

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