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dc.contributor.authorBoschi, Tommaso
dc.date.accessioned2020-11-16T15:47:06Z
dc.date.available2020-11-16T15:47:06Z
dc.date.issued2020
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/68333
dc.descriptionPhD Thesisen_US
dc.description.abstractWe are living a pivotal moment for neutrino physics. A new generation of experiments is about to begin and will extend our understanding of neutrinos. Very large scale experiments, like Hyper-Kamiokande, will collect unprecedented statistics and will constrain oscillation parameters to high precision: the CP violation phase, the octant of 23, and the mass hierarchy are likely to be determined. Many are the experimental difficulties behind a successful megaton water Cherenkov detector, but improvements in photodetection technologies luckily allow such an ambitious project. One of the most important challenges is to keep systematical uncertainties under control, so as they do not dominate over statistical errors. Assessing the impact of the systematics on the overall sensitivity of the experiment is a fundamental requirement to the final success of Hyper-Kamiokande. Thanks to powerful accelerator facilities, future long baseline experiments, such as DUNE, will also explore the intensity frontier of neutrino physics and study rare phenomena. Numerous extension to the Standard Model (SM) and alternative theories have been introduced to explain neutrino masses and mixings. These new scenarios often predict new physics, the signature of which is accessible to next-generation experiments. An interesting example comes from lowscale see-saw models, which consider GeV-scale neutral leptons coupled to SM particles with suppressed mixing angles. The near detector system of DUNE is an ideal place for searches of these particles, thanks to high exposure that compensate small event rates. Current neutrino experiments have also joined this new venture; Super-Kamiokande has been extensively refurbished in view of a new phase, starting in early 2020, in which the detector will turn into a supernova observatory. This is achieved by doping the water of Super-Kamiokande with gadolinium, in order to increase the efficiency of neutron tagging up to 90 %. The use of gadolinium is a novel technique which will be adopted by many existing and planned experiments. The benefits of improved neutron tagging are not limited just to supernova neutrinos, but to a plethora of other studies, such as reactor and atmospheric neutrinos or proton decay. In this thesis, all of the topics above are addressed. After a review of SM neutrino physics in Chapter 1, the gadolinium-loaded water Cherenkov technique is discussed in Chapter 2 with particular focus on Super-Kamiokande. A new technique to monitor gadolinium concentration in water using UV spectroscopy and an improved method for neutron calibration using a californium source are presented. Chapter 3 deals with CP violation in neutrino oscillation and the potential of Hyper-Kamiokande to constraining oscillation parameters. The methodology used to asses the experimental sensitivity is described in detail. First estimations are shown with the full systematic model and some of its variations are also taken into account. In Chapter 4 a possible Standard Model extension to explain neutrino masses is considered, and the phenomenology of such models is extensively studied in the context of a beam dump experiment. The prospect of the DUNE’s near detector to searches of heavy neutral lepton decays is then evaluated in Chapter 5. It is found that the DUNE ND is capable of extending current limits on these searches, reaching regions of the parameter space extremely interesting from a theoretical point of view.en_US
dc.language.isoenen_US
dc.publisherUniversity of Durham
dc.publisherQueen Mary University of London
dc.titleNew Physics and New Technologies in Next-Generation Neutrino Experiments.en_US
dc.typeThesisen_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US


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    Theses Awarded by Queen Mary University of London

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