PINGU: A Vision for Neutrino and Particle Physics at the South Pole

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6 Mton effective mass for neutrino detection with an energy threshol...

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Published in:Journal of Physics G: Nuclear and Particle Physics
Main Author: Andeen, Karen
Format: Text
Language:English
Published: e-Publications@Marquette 2017
Subjects:
Online Access:https://epublications.marquette.edu/physics_fac/163
https://doi.org/10.1088/1361-6471/44/5/054006
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spelling ftmarquetteuniv:oai:epublications.marquette.edu:physics_fac-1163 2023-06-11T04:16:47+02:00 PINGU: A Vision for Neutrino and Particle Physics at the South Pole Andeen, Karen 2017-04-07T07:00:00Z https://epublications.marquette.edu/physics_fac/163 https://doi.org/10.1088/1361-6471/44/5/054006 eng eng e-Publications@Marquette https://epublications.marquette.edu/physics_fac/163 https://doi.org/10.1088/1361-6471/44/5/054006 Physics Faculty Research and Publications neutrino oscillations atmospheric neutrinos IceCube Neutrino Observatory PINGU Physics text 2017 ftmarquetteuniv https://doi.org/10.1088/1361-6471/44/5/054006 2023-05-08T06:35:41Z The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6 Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60 000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters and , including the octant of for a wide range of values, and determine the neutrino mass ordering at median significance within five years of operation. PINGU's high precision measurement of the rate of appearance will provide essential tests of the unitarity of the 3 × 3 PMNS neutrino mixing matrix. PINGU will also improve the sensitivity of searches for low mass dark matter in the Sun, use neutrino tomography to directly probe the composition of the Earth's core, and improve IceCube's sensitivity to neutrinos from Galactic supernovae. Reoptimization of the PINGU design has permitted substantial reduction in both cost and logistical requirements while delivering performance nearly identical to configurations previously studied. Text South pole Marquette University: e-Publications@Marquette Pingu ENVELOPE(-52.017,-52.017,67.067,67.067) South Pole Journal of Physics G: Nuclear and Particle Physics 44 5 054006
institution Open Polar
collection Marquette University: e-Publications@Marquette
op_collection_id ftmarquetteuniv
language English
topic neutrino oscillations
atmospheric neutrinos
IceCube Neutrino Observatory
PINGU
Physics
spellingShingle neutrino oscillations
atmospheric neutrinos
IceCube Neutrino Observatory
PINGU
Physics
Andeen, Karen
PINGU: A Vision for Neutrino and Particle Physics at the South Pole
topic_facet neutrino oscillations
atmospheric neutrinos
IceCube Neutrino Observatory
PINGU
Physics
description The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6 Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60 000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters and , including the octant of for a wide range of values, and determine the neutrino mass ordering at median significance within five years of operation. PINGU's high precision measurement of the rate of appearance will provide essential tests of the unitarity of the 3 × 3 PMNS neutrino mixing matrix. PINGU will also improve the sensitivity of searches for low mass dark matter in the Sun, use neutrino tomography to directly probe the composition of the Earth's core, and improve IceCube's sensitivity to neutrinos from Galactic supernovae. Reoptimization of the PINGU design has permitted substantial reduction in both cost and logistical requirements while delivering performance nearly identical to configurations previously studied.
format Text
author Andeen, Karen
author_facet Andeen, Karen
author_sort Andeen, Karen
title PINGU: A Vision for Neutrino and Particle Physics at the South Pole
title_short PINGU: A Vision for Neutrino and Particle Physics at the South Pole
title_full PINGU: A Vision for Neutrino and Particle Physics at the South Pole
title_fullStr PINGU: A Vision for Neutrino and Particle Physics at the South Pole
title_full_unstemmed PINGU: A Vision for Neutrino and Particle Physics at the South Pole
title_sort pingu: a vision for neutrino and particle physics at the south pole
publisher e-Publications@Marquette
publishDate 2017
url https://epublications.marquette.edu/physics_fac/163
https://doi.org/10.1088/1361-6471/44/5/054006
long_lat ENVELOPE(-52.017,-52.017,67.067,67.067)
geographic Pingu
South Pole
geographic_facet Pingu
South Pole
genre South pole
genre_facet South pole
op_source Physics Faculty Research and Publications
op_relation https://epublications.marquette.edu/physics_fac/163
https://doi.org/10.1088/1361-6471/44/5/054006
op_doi https://doi.org/10.1088/1361-6471/44/5/054006
container_title Journal of Physics G: Nuclear and Particle Physics
container_volume 44
container_issue 5
container_start_page 054006
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