Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector
The IceCube Neutrino Observatory is a 1 km³ detector currently taking data at the South Pole. One of the main strategies used to look for astrophysical neutrinos with IceCube is the search for a diffuse flux of high-energy neutrinos from unresolved sources. A hard energy spectrum of neutrinos from i...
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ftunivalabama:oai:ir.ua.edu:123456789/5862 2023-05-15T18:22:51+02:00 Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector Santander, Marcos 2011-10-03 http://ir.ua.edu/handle/123456789/5862 English eng http://ir.ua.edu/handle/123456789/5862 Neutrino muon pion and other elementary particles cosmic rays Ordinary neutrinos Elementary particle processes and other elementary particle detectors cosmic ray detectors text 2011 ftunivalabama 2023-01-07T16:38:59Z The IceCube Neutrino Observatory is a 1 km³ detector currently taking data at the South Pole. One of the main strategies used to look for astrophysical neutrinos with IceCube is the search for a diffuse flux of high-energy neutrinos from unresolved sources. A hard energy spectrum of neutrinos from isotropically distributed astrophysical sources could manifest itself as a detectable signal that may be differentiated from the atmospheric neutrino background by spectral measurement. This analysis uses data from the IceCube detector collected in its half completed configuration which operated between April 2008 and May 2009 to search for a diffuse flux of astrophysical muon neutrinos. A total of 12 877 upward-going candidate neutrino events have been selected for this analysis. No evidence for a diffuse flux of astrophysical muon neutrinos was found in the data set leading to a 90% C.L. upper limit on the normalization of an E⁻² astrophysical ν_μ flux of 8.9 × 10⁻⁹ GeV cm⁻² s⁻¹ sr⁻¹. The analysis is sensitive in the energy range between 35 TeV and 7 PeV. The 12 877 candidate neutrino events are consistent with atmospheric muon neutrinos measured from 332 GeV to 84 TeV and no evidence for a prompt component to the atmospheric neutrino spectrum is found. Text South pole University of Alabama Institutional Repository South Pole |
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University of Alabama Institutional Repository |
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ftunivalabama |
language |
English |
topic |
Neutrino muon pion and other elementary particles cosmic rays Ordinary neutrinos Elementary particle processes and other elementary particle detectors cosmic ray detectors |
spellingShingle |
Neutrino muon pion and other elementary particles cosmic rays Ordinary neutrinos Elementary particle processes and other elementary particle detectors cosmic ray detectors Santander, Marcos Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector |
topic_facet |
Neutrino muon pion and other elementary particles cosmic rays Ordinary neutrinos Elementary particle processes and other elementary particle detectors cosmic ray detectors |
description |
The IceCube Neutrino Observatory is a 1 km³ detector currently taking data at the South Pole. One of the main strategies used to look for astrophysical neutrinos with IceCube is the search for a diffuse flux of high-energy neutrinos from unresolved sources. A hard energy spectrum of neutrinos from isotropically distributed astrophysical sources could manifest itself as a detectable signal that may be differentiated from the atmospheric neutrino background by spectral measurement. This analysis uses data from the IceCube detector collected in its half completed configuration which operated between April 2008 and May 2009 to search for a diffuse flux of astrophysical muon neutrinos. A total of 12 877 upward-going candidate neutrino events have been selected for this analysis. No evidence for a diffuse flux of astrophysical muon neutrinos was found in the data set leading to a 90% C.L. upper limit on the normalization of an E⁻² astrophysical ν_μ flux of 8.9 × 10⁻⁹ GeV cm⁻² s⁻¹ sr⁻¹. The analysis is sensitive in the energy range between 35 TeV and 7 PeV. The 12 877 candidate neutrino events are consistent with atmospheric muon neutrinos measured from 332 GeV to 84 TeV and no evidence for a prompt component to the atmospheric neutrino spectrum is found. |
format |
Text |
author |
Santander, Marcos |
author_facet |
Santander, Marcos |
author_sort |
Santander, Marcos |
title |
Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector |
title_short |
Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector |
title_full |
Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector |
title_fullStr |
Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector |
title_full_unstemmed |
Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-string Detector |
title_sort |
search for a diffuse flux of astrophysical muon neutrinos with the icecube 40-string detector |
publishDate |
2011 |
url |
http://ir.ua.edu/handle/123456789/5862 |
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South Pole |
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South Pole |
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South pole |
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South pole |
op_relation |
http://ir.ua.edu/handle/123456789/5862 |
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1766202258228248576 |