Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004
The Antarctic Muon and Neutrino Detector Array (AMANDA) is a Cherenkov detector deployed in the Antarctic ice cap at the South Pole. The carged-current interaction of high-energy electron or tau neutrinos, as well as the neutral-current interactions of neutrinos of any flavor, can produce isolated e...
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Universidad Nacional Autonoma de Mexico
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ftdesyvdb:oai:bib-pubdb1.desy.de:83072 2023-05-15T13:50:17+02:00 Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004 Tarasova, O. Kowalski, M. Walter, M. IceCube Collaboration DE 2007 https://bib-pubdb1.desy.de/record/83072 https://bib-pubdb1.desy.de/search?p=id:%22PHPPUBDB-5455%22 eng eng Universidad Nacional Autonoma de Mexico info:eu-repo/semantics/altIdentifier/arxiv/arXiv:0711.0353 https://bib-pubdb1.desy.de/record/83072 https://bib-pubdb1.desy.de/search?p=id:%22PHPPUBDB-5455%22 info:eu-repo/semantics/openAccess Ciudad de Mexico : Universidad Nacional Autonoma de Mexico 83-86 (2007). 30th International Cosmic Ray Conference , ICRC2007, Merida, Mexico, 2007-07-03 - 2007-07-11 info:eu-repo/semantics/report info:eu-repo/semantics/publishedVersion 2007 ftdesyvdb 2022-06-30T20:06:53Z The Antarctic Muon and Neutrino Detector Array (AMANDA) is a Cherenkov detector deployed in the Antarctic ice cap at the South Pole. The carged-current interaction of high-energy electron or tau neutrinos, as well as the neutral-current interactions of neutrinos of any flavor, can produce isolated electromagnetic or hadronic cascades. There are several advantages associated with the cascade channel in the search for a "diffuse" flux of astrophysical neutrinos. The energy resolution of AMANDA allows us to distinguish between a hard astrophysical spectrum and a soft atmospheric spectrum. In addition, the flux of atmospheric electron neutrinos is lower ba an order of magnitude relative to atmospheric nuon neutrinos, while the background from downward-going atmospheric muons can be suppressed due to their track-like topology. The low background in this channel allows us to attain 4π acceptance above energies of ∼ 50 TeV. We present the analysis of AMANDA data collected during 2000-2004. Compared to our previous analysis, this data set is a factor of five larg er, resulting in a correspondingly improved sensitivity for the flux of astrophysical neutrinos. Report Antarc* Antarctic Ice cap South pole South pole DESY Publication Database (PUBDB) Antarctic The Antarctic South Pole |
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Open Polar |
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DESY Publication Database (PUBDB) |
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language |
English |
description |
The Antarctic Muon and Neutrino Detector Array (AMANDA) is a Cherenkov detector deployed in the Antarctic ice cap at the South Pole. The carged-current interaction of high-energy electron or tau neutrinos, as well as the neutral-current interactions of neutrinos of any flavor, can produce isolated electromagnetic or hadronic cascades. There are several advantages associated with the cascade channel in the search for a "diffuse" flux of astrophysical neutrinos. The energy resolution of AMANDA allows us to distinguish between a hard astrophysical spectrum and a soft atmospheric spectrum. In addition, the flux of atmospheric electron neutrinos is lower ba an order of magnitude relative to atmospheric nuon neutrinos, while the background from downward-going atmospheric muons can be suppressed due to their track-like topology. The low background in this channel allows us to attain 4π acceptance above energies of ∼ 50 TeV. We present the analysis of AMANDA data collected during 2000-2004. Compared to our previous analysis, this data set is a factor of five larg er, resulting in a correspondingly improved sensitivity for the flux of astrophysical neutrinos. |
format |
Report |
author |
Tarasova, O. Kowalski, M. Walter, M. IceCube Collaboration |
spellingShingle |
Tarasova, O. Kowalski, M. Walter, M. IceCube Collaboration Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004 |
author_facet |
Tarasova, O. Kowalski, M. Walter, M. IceCube Collaboration |
author_sort |
Tarasova, O. |
title |
Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004 |
title_short |
Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004 |
title_full |
Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004 |
title_fullStr |
Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004 |
title_full_unstemmed |
Search for Neutrino-Induced Cacscades with AMANDA Data Taken in 2000-2004 |
title_sort |
search for neutrino-induced cacscades with amanda data taken in 2000-2004 |
publisher |
Universidad Nacional Autonoma de Mexico |
publishDate |
2007 |
url |
https://bib-pubdb1.desy.de/record/83072 https://bib-pubdb1.desy.de/search?p=id:%22PHPPUBDB-5455%22 |
op_coverage |
DE |
geographic |
Antarctic The Antarctic South Pole |
geographic_facet |
Antarctic The Antarctic South Pole |
genre |
Antarc* Antarctic Ice cap South pole South pole |
genre_facet |
Antarc* Antarctic Ice cap South pole South pole |
op_source |
Ciudad de Mexico : Universidad Nacional Autonoma de Mexico 83-86 (2007). 30th International Cosmic Ray Conference , ICRC2007, Merida, Mexico, 2007-07-03 - 2007-07-11 |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/arXiv:0711.0353 https://bib-pubdb1.desy.de/record/83072 https://bib-pubdb1.desy.de/search?p=id:%22PHPPUBDB-5455%22 |
op_rights |
info:eu-repo/semantics/openAccess |
_version_ |
1766253314973892608 |