Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam

There are recent considerations to increase the photomultiplier density in the IceCube detector array beyond that of DeepCore, which will lead to a lower detection threshold and a huge fiducial mass for the neutrino detection. This initiative is known as "Phased IceCube Next Generation Upgrade&...

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Published in:Journal of High Energy Physics
Main Authors: Tang, Jian, Winter, Walter
Language:English
Published: 2011
Subjects:
Online Access:https://doi.org/10.1007/JHEP02(2012)028
http://cds.cern.ch/record/1393996
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spelling ftcern:oai:cds.cern.ch:1393996 2023-05-15T18:23:05+02:00 Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam Tang, Jian Winter, Walter 2011-10-28 https://doi.org/10.1007/JHEP02(2012)028 http://cds.cern.ch/record/1393996 eng eng doi:10.1007/JHEP02(2012)028 http://cds.cern.ch/record/1393996 arXiv:1110.5908 IDS-NF-031 oai:cds.cern.ch:1393996 Particle Physics - Phenomenology 2011 ftcern https://doi.org/10.1007/JHEP02(2012)028 2018-07-28T09:54:23Z There are recent considerations to increase the photomultiplier density in the IceCube detector array beyond that of DeepCore, which will lead to a lower detection threshold and a huge fiducial mass for the neutrino detection. This initiative is known as "Phased IceCube Next Generation Upgrade" (PINGU). We discuss the possibility to send a neutrino beam from one of the major accelerator laboratories in the Northern hemisphere to such a detector. Such an experiment would be unique in the sense that it would be the only neutrino beam where the baseline crosses the Earth's core. We study the detector requirements for a beta beam, a neutrino factory beam, and a superbeam, where we consider both the cases of small theta_13 and large theta_13, as suggested by the recent T2K hint. We illustrate that a flavor-clean beta beam best suits the requirements of such a detector, in particular, that PINGU may replace a magic baseline detector for small values of theta_13 -- even in the absence of any energy resolution capability. For large theta_13, however, a single-baseline beta beam experiment cannot compete if it is constrained by the CERN-SPS. For a neutrino factory, because of the missing charge identification possibility in the detector, a very good energy resolution is required. If this can be achieved, especially a low energy neutrino factory, which does not suffer from the tau contamination, may be an interesting option for large theta_13. For the superbeam, where we use the LBNE beam as a reference, electron neutrino flavor identification and statistics are two of the main limitations. Finally, we demonstrate that, at least in principle, neutrino factory and superbeam can measure the density of the Earth's core to the sub-percent level for sin^2 2theta_13 larger than 0.01. Other/Unknown Material South pole CERN Document Server (CDS) Pingu ENVELOPE(-52.017,-52.017,67.067,67.067) South Pole Journal of High Energy Physics 2012 2
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Particle Physics - Phenomenology
spellingShingle Particle Physics - Phenomenology
Tang, Jian
Winter, Walter
Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam
topic_facet Particle Physics - Phenomenology
description There are recent considerations to increase the photomultiplier density in the IceCube detector array beyond that of DeepCore, which will lead to a lower detection threshold and a huge fiducial mass for the neutrino detection. This initiative is known as "Phased IceCube Next Generation Upgrade" (PINGU). We discuss the possibility to send a neutrino beam from one of the major accelerator laboratories in the Northern hemisphere to such a detector. Such an experiment would be unique in the sense that it would be the only neutrino beam where the baseline crosses the Earth's core. We study the detector requirements for a beta beam, a neutrino factory beam, and a superbeam, where we consider both the cases of small theta_13 and large theta_13, as suggested by the recent T2K hint. We illustrate that a flavor-clean beta beam best suits the requirements of such a detector, in particular, that PINGU may replace a magic baseline detector for small values of theta_13 -- even in the absence of any energy resolution capability. For large theta_13, however, a single-baseline beta beam experiment cannot compete if it is constrained by the CERN-SPS. For a neutrino factory, because of the missing charge identification possibility in the detector, a very good energy resolution is required. If this can be achieved, especially a low energy neutrino factory, which does not suffer from the tau contamination, may be an interesting option for large theta_13. For the superbeam, where we use the LBNE beam as a reference, electron neutrino flavor identification and statistics are two of the main limitations. Finally, we demonstrate that, at least in principle, neutrino factory and superbeam can measure the density of the Earth's core to the sub-percent level for sin^2 2theta_13 larger than 0.01.
author Tang, Jian
Winter, Walter
author_facet Tang, Jian
Winter, Walter
author_sort Tang, Jian
title Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam
title_short Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam
title_full Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam
title_fullStr Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam
title_full_unstemmed Requirements for a New Detector at the South Pole Receiving an Accelerator Neutrino Beam
title_sort requirements for a new detector at the south pole receiving an accelerator neutrino beam
publishDate 2011
url https://doi.org/10.1007/JHEP02(2012)028
http://cds.cern.ch/record/1393996
long_lat ENVELOPE(-52.017,-52.017,67.067,67.067)
geographic Pingu
South Pole
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genre South pole
genre_facet South pole
op_relation doi:10.1007/JHEP02(2012)028
http://cds.cern.ch/record/1393996
arXiv:1110.5908
IDS-NF-031
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op_doi https://doi.org/10.1007/JHEP02(2012)028
container_title Journal of High Energy Physics
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container_issue 2
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