Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range

The IceCube neutrino observatory is a large-scale particle physics experiment at the South Pole. IceCube consists of a series of sensors embedded in the ice that detect the Cherenkov radiation produced when a neutrino interacts with the ice. Given its great success and reliability, the IceCube detec...

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Bibliographic Details
Main Author: Lozano Mariscal, Cristian Jesús
Other Authors: Kappes, Alexander, Weinheimer, Christian
Format: Doctoral or Postdoctoral Thesis
Language:English
Published: Zenodo 2023
Subjects:
Ice
Online Access:https://doi.org/10.5281/zenodo.8107177
id ftzenodo:oai:zenodo.org:8107177
record_format openpolar
spelling ftzenodo:oai:zenodo.org:8107177 2024-09-15T18:36:55+00:00 Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range Lozano Mariscal, Cristian Jesús Kappes, Alexander Weinheimer, Christian 2023-05-05 https://doi.org/10.5281/zenodo.8107177 eng eng Zenodo https://doi.org/10.5281/zenodo.8107176 https://doi.org/10.5281/zenodo.8107177 oai:zenodo.org:8107177 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode IceCube Upgrade IceCube-Gen2 Neutrinos Supernova Calibration Ice Compact binary mergers info:eu-repo/semantics/doctoralThesis 2023 ftzenodo https://doi.org/10.5281/zenodo.810717710.5281/zenodo.8107176 2024-07-27T07:41:40Z The IceCube neutrino observatory is a large-scale particle physics experiment at the South Pole. IceCube consists of a series of sensors embedded in the ice that detect the Cherenkov radiation produced when a neutrino interacts with the ice. Given its great success and reliability, the IceCube detector is being expanded through two extension projects: IceCube Upgrade and IceCube-Gen2. The IceCube Upgrade project aims to install ∼700 new optical modules in a dense configuration in the existing IceCube volume to detect low-energy neutrinos; construction is planned for the Australian summer of 2025-2026. IceCube-Gen2 envisions an expansion of the instrumented volume from 1 to 8 km 3 with new optical modules. Construction is scheduled to begin shortly after the completion of IceCube Upgrade. This expansion will allow IceCube to significantly increase its detection rate of cosmic high-energy neutrinos and further improve our understandingof the universe. This thesis presents the results of simulation studies that evaluate the potential of future detector extensions for a number of topics. The first study focuses on the detection of low-energy neutrinos released during a core collapse supernova (CCSN) with the new IceCube-Gen2 detector when equipped with multi-PMT digital optical modules (mDOMs). It is shown that CCSNe can be detected up to distances of ∼250 kpc with a false detection rate of less than one per century. The second study examines the calibration of bubble column parameters in IceCube Upgrade. The bubble column, a region of frozen ice in the middle of the strings with poorer optical properties than the bulk ice, is a significant source of systematic uncertainties in the current detector, and determining its properties will benefit not only the future detector but also allow improved re-analyzes of existing data. This study shows that its properties can be reconstructed with high precision by lining up two adjacent mDOMs and flashing the LEDs in one of them. The last study investigates the sensitivity of ... Doctoral or Postdoctoral Thesis South pole Zenodo
institution Open Polar
collection Zenodo
op_collection_id ftzenodo
language English
topic IceCube
Upgrade
IceCube-Gen2
Neutrinos
Supernova
Calibration
Ice
Compact binary mergers
spellingShingle IceCube
Upgrade
IceCube-Gen2
Neutrinos
Supernova
Calibration
Ice
Compact binary mergers
Lozano Mariscal, Cristian Jesús
Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range
topic_facet IceCube
Upgrade
IceCube-Gen2
Neutrinos
Supernova
Calibration
Ice
Compact binary mergers
description The IceCube neutrino observatory is a large-scale particle physics experiment at the South Pole. IceCube consists of a series of sensors embedded in the ice that detect the Cherenkov radiation produced when a neutrino interacts with the ice. Given its great success and reliability, the IceCube detector is being expanded through two extension projects: IceCube Upgrade and IceCube-Gen2. The IceCube Upgrade project aims to install ∼700 new optical modules in a dense configuration in the existing IceCube volume to detect low-energy neutrinos; construction is planned for the Australian summer of 2025-2026. IceCube-Gen2 envisions an expansion of the instrumented volume from 1 to 8 km 3 with new optical modules. Construction is scheduled to begin shortly after the completion of IceCube Upgrade. This expansion will allow IceCube to significantly increase its detection rate of cosmic high-energy neutrinos and further improve our understandingof the universe. This thesis presents the results of simulation studies that evaluate the potential of future detector extensions for a number of topics. The first study focuses on the detection of low-energy neutrinos released during a core collapse supernova (CCSN) with the new IceCube-Gen2 detector when equipped with multi-PMT digital optical modules (mDOMs). It is shown that CCSNe can be detected up to distances of ∼250 kpc with a false detection rate of less than one per century. The second study examines the calibration of bubble column parameters in IceCube Upgrade. The bubble column, a region of frozen ice in the middle of the strings with poorer optical properties than the bulk ice, is a significant source of systematic uncertainties in the current detector, and determining its properties will benefit not only the future detector but also allow improved re-analyzes of existing data. This study shows that its properties can be reconstructed with high precision by lining up two adjacent mDOMs and flashing the LEDs in one of them. The last study investigates the sensitivity of ...
author2 Kappes, Alexander
Weinheimer, Christian
format Doctoral or Postdoctoral Thesis
author Lozano Mariscal, Cristian Jesús
author_facet Lozano Mariscal, Cristian Jesús
author_sort Lozano Mariscal, Cristian Jesús
title Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range
title_short Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range
title_full Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range
title_fullStr Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range
title_full_unstemmed Ice calibration studies for IceCube Upgrade with multi-PMT optical modules, and studies of the sensitivity of future IceCube extensions to astrophysical neutrinos in the MeV and GeV range
title_sort ice calibration studies for icecube upgrade with multi-pmt optical modules, and studies of the sensitivity of future icecube extensions to astrophysical neutrinos in the mev and gev range
publisher Zenodo
publishDate 2023
url https://doi.org/10.5281/zenodo.8107177
genre South pole
genre_facet South pole
op_relation https://doi.org/10.5281/zenodo.8107176
https://doi.org/10.5281/zenodo.8107177
oai:zenodo.org:8107177
op_rights info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
op_doi https://doi.org/10.5281/zenodo.810717710.5281/zenodo.8107176
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