Measurement of neutron-proton capture in the SNO+ water phase
Abstract:
The SNO+ experiment collected data as a low-threshold water Cherenkov detector from September 2017 to July 2019. Measurements of the 2.2-MeV $\gamma$ produced by neutron capture on hydrogen have been made using an Am-Be calibration source, for which a large fraction of emitted neutrons are produced simultaneously with a 4.4-MeV $\gamma$. Analysis of the delayed coincidence between the 4.4-MeV $\gamma$ and the 2.2-MeV capture $\gamma$ revealed a neutron detection efficiency that is centered around 50% and varies at the level of 1% across the inner region of the detector, which to our knowledge is the highest efficiency achieved among pure water Cherenkov detectors. In addition, the neutron capture time constant was measured and converted to a thermal neutron-proton capture cross section of $336.3^{+1.2}_{-1.5}$ mb.Measurement of oscillations in solar boron-8 neutrinos and studies of optical scattering in the SNO+ detector
Abstract:
SNO+ is a large-scale liquid scintillator experiment based in Sudbury, Canada, capable of probing many aspects of neutrinos. One major property of interest is the neutrino’s ability to oscillate between different flavours, an indirect demonstration that neutrinos must have mass.
This thesis performs the first ever measurement of oscillations from 8B solar neutrinos in the scintillator phase of SNO+. Assuming the current global fit flux of 8 B solar neutrinos, the neutrino oscillation parameter theta_12 was measured to be 38.9 degrees +8.0-7.9 degrees, using an initial 80.6 days of data. This result is consistent with the current global fit result of 33.44 degrees +0.77-0.74 degrees. A sensitivity study indicates that the precision of this result is capable of improving by at least a factor of two within two years of livetime.
On top of this, substantial improvements were made to all aspects of the optical calibration system known as SMELLIE. This is a series of optical-wavelength lasers whose light is emitted from optical fibres attached to the edge of the SNO+ detector. By developing a new analysis, this system was able to measure the scintillator extinction lengths as a function of wavelength and time in-situ for the first time. A new analysis was also built and demonstrated to observe changes in scattering and scintillator re-emission properties of the scintillator as a function of time and wavelength. Alongside this, major upgrades were made to both the hardware and simulation of the SMELLIE system, enabling higher-quality data to be taken, and simulations to be made with much greater speed.