Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data

We report on a search for extremely-high energy neutrinos with energies greater than 106GeV using the data taken with the IceCube detector at the South Pole. The data was collected between April 2008 and May 2009 with the half-completed IceCube array. The absence of signal candidate events in the sa...

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Published in:Physical Review D
Main Authors: Abbasi, R., Hill, G.
Format: Article in Journal/Newspaper
Language:English
Published: American Physical Soc 2011
Subjects:
Online Access:http://hdl.handle.net/2440/76714
https://doi.org/10.1103/PhysRevD.83.092003
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spelling ftunivadelaidedl:oai:digital.library.adelaide.edu.au:2440/76714 2023-12-24T10:24:54+01:00 Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data Abbasi, R. Hill, G. 2011 application/pdf http://hdl.handle.net/2440/76714 https://doi.org/10.1103/PhysRevD.83.092003 en eng American Physical Soc Physical Review D: Particles, Fields, Gravitation and Cosmology, 2011; 83(9):092003:1-092003:9 1550-7998 1550-2368 http://hdl.handle.net/2440/76714 doi:10.1103/PhysRevD.83.092003 © 2011 American Physical Society http://dx.doi.org/10.1103/physrevd.83.092003 Journal article 2011 ftunivadelaidedl https://doi.org/10.1103/PhysRevD.83.09200310.1103/physrevd.83.092003 2023-11-27T23:26:28Z We report on a search for extremely-high energy neutrinos with energies greater than 106GeV using the data taken with the IceCube detector at the South Pole. The data was collected between April 2008 and May 2009 with the half-completed IceCube array. The absence of signal candidate events in the sample of 333.5 days of live time significantly improves model-independent limits from previous searches and allows to place a limit on the diffuse flux of cosmic neutrinos with an E-2 spectrum in the energy range 2.0×106-6.3×109GeV to a level of E2φ≤3.6×10 -8GeVcm-2sec-1sr-1. © 2011 American Physical Society. R. Abbasi . G. C. Hill . et al. IceCube Collaboration Article in Journal/Newspaper South pole The University of Adelaide: Digital Library South Pole Physical Review D 83 9
institution Open Polar
collection The University of Adelaide: Digital Library
op_collection_id ftunivadelaidedl
language English
description We report on a search for extremely-high energy neutrinos with energies greater than 106GeV using the data taken with the IceCube detector at the South Pole. The data was collected between April 2008 and May 2009 with the half-completed IceCube array. The absence of signal candidate events in the sample of 333.5 days of live time significantly improves model-independent limits from previous searches and allows to place a limit on the diffuse flux of cosmic neutrinos with an E-2 spectrum in the energy range 2.0×106-6.3×109GeV to a level of E2φ≤3.6×10 -8GeVcm-2sec-1sr-1. © 2011 American Physical Society. R. Abbasi . G. C. Hill . et al. IceCube Collaboration
format Article in Journal/Newspaper
author Abbasi, R.
Hill, G.
spellingShingle Abbasi, R.
Hill, G.
Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data
author_facet Abbasi, R.
Hill, G.
author_sort Abbasi, R.
title Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data
title_short Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data
title_full Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data
title_fullStr Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data
title_full_unstemmed Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data
title_sort constraints on the extremely-high energy cosmic neutrino flux with the icecube 2008-2009 data
publisher American Physical Soc
publishDate 2011
url http://hdl.handle.net/2440/76714
https://doi.org/10.1103/PhysRevD.83.092003
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source http://dx.doi.org/10.1103/physrevd.83.092003
op_relation Physical Review D: Particles, Fields, Gravitation and Cosmology, 2011; 83(9):092003:1-092003:9
1550-7998
1550-2368
http://hdl.handle.net/2440/76714
doi:10.1103/PhysRevD.83.092003
op_rights © 2011 American Physical Society
op_doi https://doi.org/10.1103/PhysRevD.83.09200310.1103/physrevd.83.092003
container_title Physical Review D
container_volume 83
container_issue 9
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