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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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 |
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University of Canterbury, Christchurch: UC Research Repository |
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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 |
_version_ |
1766202811984379904 |