Identifying cosmic ray induced cascade events with IceTop

IceCube is the largest neutrino detector in the world. It consists of an array of photomultiplier tubes installed throughout a cubic kilometre of ice below the surface at the South Pole. These photomultiplier tubes detect the Cherenkov radiation from neutrino-nucleon interactions. IceTop is the surf...

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Main Author: Munawar, Kiran
Format: Other/Unknown Material
Language:English
Published: University of Canterbury 2017
Subjects:
Online Access:http://hdl.handle.net/10092/14940
https://doi.org/10.26021/8983
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spelling ftunivcanter:oai:ir.canterbury.ac.nz:10092/14940 2023-05-15T18:23:16+02:00 Identifying cosmic ray induced cascade events with IceTop Munawar, Kiran 2017 application/pdf http://hdl.handle.net/10092/14940 https://doi.org/10.26021/8983 English en eng University of Canterbury http://hdl.handle.net/10092/14940 http://dx.doi.org/10.26021/8983 All Rights Reserved https://canterbury.libguides.com/rights/theses Theses / Dissertations 2017 ftunivcanter https://doi.org/10.26021/8983 2022-09-08T13:42:13Z IceCube is the largest neutrino detector in the world. It consists of an array of photomultiplier tubes installed throughout a cubic kilometre of ice below the surface at the South Pole. These photomultiplier tubes detect the Cherenkov radiation from neutrino-nucleon interactions. IceTop is the surface component of IceCube neutrino observatory and is used to study Cosmic Ray Extensive Air Showers (EAS). The goal of IceCube is to investigate astophysical neutrinos. However the majority of events recorded by IceCube are background events caused by cosmic rays interacting in the Earth's atmosphere. This thesis is concerned with developing a technique to veto the background events from the IceCube experimental data using the IceTop surface array. Four original studies were performed. In the rst study the output of a cosmic-ray air shower simulation code was compared with real events detected by IceCube and IceTop. It was found that the simulation code performed well, although in some cases the actual number of hits detected in IceTop ws greater than predicted. However as far as assessing the ability of IceTop as a veto this means our estimates will be conservative which would mean that the veto would be more e ective than estimated. In the second study the cosmic-ray simulation code was used to investigate the scope of background events which might be able to vetoed using the IceTop array and the energies and zenith angles where the veto would be e ective were given. The appropriate time window for deciding whether an IceTop hit was related to an event detected in the IceCube detector was investigated in the third study and was found to be -500 ns to 800 ns relative to the timing of the IceCube event. In the fourth study, the nal sample of a published IceCube cascade analysis was examined to determine whether there were any related hits in the IceTop array. 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 IceCube is the largest neutrino detector in the world. It consists of an array of photomultiplier tubes installed throughout a cubic kilometre of ice below the surface at the South Pole. These photomultiplier tubes detect the Cherenkov radiation from neutrino-nucleon interactions. IceTop is the surface component of IceCube neutrino observatory and is used to study Cosmic Ray Extensive Air Showers (EAS). The goal of IceCube is to investigate astophysical neutrinos. However the majority of events recorded by IceCube are background events caused by cosmic rays interacting in the Earth's atmosphere. This thesis is concerned with developing a technique to veto the background events from the IceCube experimental data using the IceTop surface array. Four original studies were performed. In the rst study the output of a cosmic-ray air shower simulation code was compared with real events detected by IceCube and IceTop. It was found that the simulation code performed well, although in some cases the actual number of hits detected in IceTop ws greater than predicted. However as far as assessing the ability of IceTop as a veto this means our estimates will be conservative which would mean that the veto would be more e ective than estimated. In the second study the cosmic-ray simulation code was used to investigate the scope of background events which might be able to vetoed using the IceTop array and the energies and zenith angles where the veto would be e ective were given. The appropriate time window for deciding whether an IceTop hit was related to an event detected in the IceCube detector was investigated in the third study and was found to be -500 ns to 800 ns relative to the timing of the IceCube event. In the fourth study, the nal sample of a published IceCube cascade analysis was examined to determine whether there were any related hits in the IceTop array.
format Other/Unknown Material
author Munawar, Kiran
spellingShingle Munawar, Kiran
Identifying cosmic ray induced cascade events with IceTop
author_facet Munawar, Kiran
author_sort Munawar, Kiran
title Identifying cosmic ray induced cascade events with IceTop
title_short Identifying cosmic ray induced cascade events with IceTop
title_full Identifying cosmic ray induced cascade events with IceTop
title_fullStr Identifying cosmic ray induced cascade events with IceTop
title_full_unstemmed Identifying cosmic ray induced cascade events with IceTop
title_sort identifying cosmic ray induced cascade events with icetop
publisher University of Canterbury
publishDate 2017
url http://hdl.handle.net/10092/14940
https://doi.org/10.26021/8983
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation http://hdl.handle.net/10092/14940
http://dx.doi.org/10.26021/8983
op_rights All Rights Reserved
https://canterbury.libguides.com/rights/theses
op_doi https://doi.org/10.26021/8983
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