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dc.contributor.authorGhaith, Muad
dc.contributor.otherQueen's University (Kingston, Ont.). Theses (Queen's University (Kingston, Ont.))en
dc.date.accessioned2017-04-19T20:48:30Z
dc.date.available2017-04-19T20:48:30Z
dc.identifier.urihttp://hdl.handle.net/1974/15657
dc.description.abstractA significant evidence from galaxies and astrophysical observations, suggests that ~ 85% of the matter in our Universe is invisible matter. The observations of the so-called “dark matter” suggest that it consists of non-relativistic, non-baryonic particles, which seldom interact with baryonic matter, or with each other. Many experiments are searching for dark matter, each of which is based on a particular dark matter candidate. Weakly Interacting Massive Particles (WIMPs) are one of the well-motivated candidates for dark matter. So far, no answers were provided by the Standard Model of particle physics to the dark matter puzzle. The Super Cryogenic Dark Matter Search experiment (SuperCDMS) is considered one of the pioneer experiments in the direct search for WIMPs. It is based primarily on deploying germanium and silicon detectors at cryogenic temperatures to search for direct WIMP-nucleus elastic scattering interaction through which lattice vibrations are generated and sensed in one of the coldest detectors ever built. The new phase of SuperCDMS experiment at SNOLAB is aiming to be sensitive to the lower WIMP mass scale. Therefore, a lower background and detector threshold energy is a necessity, and the detectors need to be calibrated and tested for the new proposed sensitivity. The tests include high bias voltages, which are required to increase the gain in signal-to-noise ratio and to allow for the detection of low energy events using the phonon signal. However, the upper limit and polarity for the bias voltage need further studies in order to understand the variation of the detector’s response to high voltage. Therefore, we performed the breakdown measurement (chapter 4) at Queen’s Test Facility. Moreover, detectors have to be calibrated before being utilized in measuring low energy interactions, and that is what lead to the use of infrared photons. Once we can calibrate and understand the behavior of infrared photons in germanium detectors, they can be utilized in calibrating germanium detectors at the lower energy scale. Therefore, we performed the infrared calibration measurement which represents the bulk of the work in my thesis.en_US
dc.language.isoenen_US
dc.relation.ispartofseriesCanadian thesesen
dc.rightsCC0 1.0 Universal*
dc.rightsQueen's University's Thesis/Dissertation Non-Exclusive License for Deposit to QSpace and Library and Archives Canadaen
dc.rightsProQuest PhD and Master's Theses International Dissemination Agreementen
dc.rightsIntellectual Property Guidelines at Queen's Universityen
dc.rightsCopying and Preserving Your Thesisen
dc.rightsThis publication is made available by the authority of the copyright owner solely for the purpose of private study and research and may not be copied or reproduced except as permitted by the copyright laws without written authority from the copyright owner.en
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/*
dc.subjectDark Matteren_US
dc.subjectCryogenic Detectorsen_US
dc.subjectSuperCDMSen_US
dc.subjectWIMPen_US
dc.titleCalibration of Infrared Photons in Cryogenic Germanium Detectorsen_US
dc.typeThesisen_US
dc.description.degreeMaster of Scienceen_US
dc.contributor.supervisorRau, Wolfgang
dc.contributor.departmentPhysics, Engineering Physics and Astronomyen_US


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