Characterising the optical response of the SNO+ detector

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Title: Characterising the optical response of the SNO+ detector
Authors: Stainforth, R.
Committee Members: McCauley, N.
Summary: SNO+ is a liquid scintillator based neutrino experiment located 2039 m underground in VALE's Creighton mine, Lively, Ontario, CA. It is a re-purposing of the original Cherenkov detector used in the SNO experiment to study neutrino oscillations. The advent of neutrino oscillations has revealed that neutrinos have a small yet non-zero mass. However, the nature of this mass has yet to be determined. It is possible that the neutrino is its own anti-particle, a Majorana fermion. If so, such particles necessitate lepton number violating processes such as neutrinoless double beta decay. SNO+ intends to search for the neutrinoless double beta decay of Te-130. Other physics objectives include the study of low-energy solar neutrinos, reactor anti-neutrinos, geo-neutrinos and sensitivity to nucleon decay and supernova neutrinos. To fulfil these objectives, SNO+ will operate over three detector phases; water, scintillator and tellurium (loading of the scintillator with tellurium). Prior to each phase, the experiment will undergo a full detector calibration. This includes an optical calibration that seeks to characterise the optical response of the detector using two types of in-situ light sources; one of these is called the laserball. The laserball provides a pulsed, near-isotropic light distribution throughout the detector. Laserball data is used in conjunction with a parameterised model that characterises the optical response; the parameters are determined using a statistical fit. This thesis presents an implementation of said model to all three phases of the SNO+ experiment. A characterisation of the optical response in water is presented using a combination of original laserball data from SNO and MC data of the SNO+ detector. Thereafter, the two scintillator based phases are considered, wherein the increased attenuation of light due to absorption and reemission introduced by the scintillator is addressed alongside a model of the scintillation time profile.
URL: https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.706838
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  Label: Title
  Group: Ti
  Data: Characterising the optical response of the SNO+ detector
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  Data: <searchLink fieldCode="AR" term="%22Stainforth%2C+R%2E%22">Stainforth, R.</searchLink>
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  Data: <searchLink fieldCode="CO" term="%22McCauley%2C+N%2E%22">McCauley, N.</searchLink>
– Name: Abstract
  Label: Summary
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  Data: SNO+ is a liquid scintillator based neutrino experiment located 2039 m underground in VALE's Creighton mine, Lively, Ontario, CA. It is a re-purposing of the original Cherenkov detector used in the SNO experiment to study neutrino oscillations. The advent of neutrino oscillations has revealed that neutrinos have a small yet non-zero mass. However, the nature of this mass has yet to be determined. It is possible that the neutrino is its own anti-particle, a Majorana fermion. If so, such particles necessitate lepton number violating processes such as neutrinoless double beta decay. SNO+ intends to search for the neutrinoless double beta decay of Te-130. Other physics objectives include the study of low-energy solar neutrinos, reactor anti-neutrinos, geo-neutrinos and sensitivity to nucleon decay and supernova neutrinos. To fulfil these objectives, SNO+ will operate over three detector phases; water, scintillator and tellurium (loading of the scintillator with tellurium). Prior to each phase, the experiment will undergo a full detector calibration. This includes an optical calibration that seeks to characterise the optical response of the detector using two types of in-situ light sources; one of these is called the laserball. The laserball provides a pulsed, near-isotropic light distribution throughout the detector. Laserball data is used in conjunction with a parameterised model that characterises the optical response; the parameters are determined using a statistical fit. This thesis presents an implementation of said model to all three phases of the SNO+ experiment. A characterisation of the optical response in water is presented using a combination of original laserball data from SNO and MC data of the SNO+ detector. Thereafter, the two scintillator based phases are considered, wherein the increased attenuation of light due to absorption and reemission introduced by the scintillator is addressed alongside a model of the scintillation time profile.
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    Languages:
      – Code: eng
        Text: English
    Subjects:
      – SubjectFull: 539.7
        Type: general
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      – TitleFull: Characterising the optical response of the SNO+ detector
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            NameFull: Stainforth, R.
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          Dates:
            – D: 01
              M: 01
              Type: published
              Y: 2016
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