Incorporating an IceTop veto for cascade events

The IceCube observatory, at the South Pole, includes an array of optical sensors deployed between 1450 and 2450 m below the surface and a surface array of cosmic ray detectors. The deep array, IceCube-InIce, is the world’s largest neutrino detector and consists of over 5000 optical sensors which det...

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Main Author: Bagherpour, Hadis
Format: Other/Unknown Material
Language:English
Published: University of Canterbury 2019
Subjects:
Online Access:http://hdl.handle.net/10092/17516
https://doi.org/10.26021/6648
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spelling ftunivcanter:oai:ir.canterbury.ac.nz:10092/17516 2023-05-15T18:23:15+02:00 Incorporating an IceTop veto for cascade events Bagherpour, Hadis 2019 application/pdf http://hdl.handle.net/10092/17516 https://doi.org/10.26021/6648 English en eng University of Canterbury http://hdl.handle.net/10092/17516 http://dx.doi.org/10.26021/6648 All Rights Reserved https://canterbury.libguides.com/rights/theses Theses / Dissertations 2019 ftunivcanter https://doi.org/10.26021/6648 2022-09-08T13:32:04Z The IceCube observatory, at the South Pole, includes an array of optical sensors deployed between 1450 and 2450 m below the surface and a surface array of cosmic ray detectors. The deep array, IceCube-InIce, is the world’s largest neutrino detector and consists of over 5000 optical sensors which detect the optical Cherenkov light emitted by the charged particles produced when neutrinos interact in the ice. Neutrinos are unique astronomical messenger particles as they can travel across the Universe without interference or being absorbed by matter. In contrast to charged particles, whose trajectories are affected by magnetic fields, neutrinos’ trajectories can be used to point back to their sources to aid the identification of particle acceleration sites. Although the main aim of IceCube-InIce is to search for astrophysical neutrinos, the majority of events recorded are background events originating from the interaction of cosmic rays in the Earth’s atmosphere. In this thesis, the use of the IceTop surface array as a veto to identify background events is investigated. The focus of this thesis is the study of the implementation of an IceTop veto within an IceCube-InIce cascade analysis. A cascade analysis focuses on selecting IceCube-InIce events where the neutrino interaction has resulted in a shower or cascade of secondary particles rather than a long-range particle. The resulting pattern of light detected across the optical sensors appears globular rather than elongated and track-like. There are two variations of cascade analyses; contained and uncontained analyses. Contained cascade analyses concentrate on events where the central point of the light pattern is well-contained within the IceCube-InIce array while the uncontained analyses focus on the remaining events. In this thesis it is shown that there is potential for an IceTop veto to be used in a way that allows other filter criteria to be relaxed in an uncontained cascade analysis in order to aid signal retention and for the veto to be used to remove ... Other/Unknown Material South pole University of Canterbury, Christchurch: UC Research Repository South Pole
institution Open Polar
collection University of Canterbury, Christchurch: UC Research Repository
op_collection_id ftunivcanter
language English
description The IceCube observatory, at the South Pole, includes an array of optical sensors deployed between 1450 and 2450 m below the surface and a surface array of cosmic ray detectors. The deep array, IceCube-InIce, is the world’s largest neutrino detector and consists of over 5000 optical sensors which detect the optical Cherenkov light emitted by the charged particles produced when neutrinos interact in the ice. Neutrinos are unique astronomical messenger particles as they can travel across the Universe without interference or being absorbed by matter. In contrast to charged particles, whose trajectories are affected by magnetic fields, neutrinos’ trajectories can be used to point back to their sources to aid the identification of particle acceleration sites. Although the main aim of IceCube-InIce is to search for astrophysical neutrinos, the majority of events recorded are background events originating from the interaction of cosmic rays in the Earth’s atmosphere. In this thesis, the use of the IceTop surface array as a veto to identify background events is investigated. The focus of this thesis is the study of the implementation of an IceTop veto within an IceCube-InIce cascade analysis. A cascade analysis focuses on selecting IceCube-InIce events where the neutrino interaction has resulted in a shower or cascade of secondary particles rather than a long-range particle. The resulting pattern of light detected across the optical sensors appears globular rather than elongated and track-like. There are two variations of cascade analyses; contained and uncontained analyses. Contained cascade analyses concentrate on events where the central point of the light pattern is well-contained within the IceCube-InIce array while the uncontained analyses focus on the remaining events. In this thesis it is shown that there is potential for an IceTop veto to be used in a way that allows other filter criteria to be relaxed in an uncontained cascade analysis in order to aid signal retention and for the veto to be used to remove ...
format Other/Unknown Material
author Bagherpour, Hadis
spellingShingle Bagherpour, Hadis
Incorporating an IceTop veto for cascade events
author_facet Bagherpour, Hadis
author_sort Bagherpour, Hadis
title Incorporating an IceTop veto for cascade events
title_short Incorporating an IceTop veto for cascade events
title_full Incorporating an IceTop veto for cascade events
title_fullStr Incorporating an IceTop veto for cascade events
title_full_unstemmed Incorporating an IceTop veto for cascade events
title_sort incorporating an icetop veto for cascade events
publisher University of Canterbury
publishDate 2019
url http://hdl.handle.net/10092/17516
https://doi.org/10.26021/6648
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation http://hdl.handle.net/10092/17516
http://dx.doi.org/10.26021/6648
op_rights All Rights Reserved
https://canterbury.libguides.com/rights/theses
op_doi https://doi.org/10.26021/6648
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