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Title: Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II

Abstract

The AMANDA-II detector, operating since 2000 in the deep ice at the geographic South Pole, has accumulated a large sample of atmospheric muon neutrinos in the 100 GeV to 10 TeV energy range. The zenith angle and energy distribution of these events can be used to search for various phenomenological signatures of quantum gravity in the neutrino sector, such as violation of Lorentz invariance or quantum decoherence. Analyzing a set of 5511 candidate neutrino events collected during 1387 days of livetime from 2000 to 2006, we find no evidence for such effects and set upper limits on violation of Lorentz invariance and quantum decoherence parameters using a maximum likelihood method. Given the absence of evidence for new flavor-changing physics, we use the same methodology to determine the conventional atmospheric muon neutrino flux above 100 GeV.

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ;  [1]
  1. Department of Physics, University of Wisconsin, Madison, Wisconsin 53706 (United States)
Publication Date:
OSTI Identifier:
21296296
Resource Type:
Journal Article
Journal Name:
Physical Review. D, Particles Fields
Additional Journal Information:
Journal Volume: 79; Journal Issue: 10; Other Information: DOI: 10.1103/PhysRevD.79.102005; (c) 2009 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0556-2821
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ANTARCTICA; ENERGY SPECTRA; FLAVOR MODEL; GEV RANGE 100-1000; ICE; LORENTZ INVARIANCE; MAXIMUM-LIKELIHOOD FIT; MUON NEUTRINOS; QUANTUM DECOHERENCE; QUANTUM GRAVITY; TEV RANGE 01-10

Citation Formats

Abbasi, R, Andeen, K, Baker, M, Berghaus, P, Boersma, D J, Braun, J, Chirkin, D, Desiati, P, Diaz-Velez, J C, Dumm, J P, Eisch, J, Finley, C, Ganugapati, R, Gladstone, L, Grullon, S, Halzen, F, Hanson, K, Hill, G C, Hoshina, K, and Jacobsen, J. Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II. United States: N. p., 2009. Web. doi:10.1103/PHYSREVD.79.102005.
Abbasi, R, Andeen, K, Baker, M, Berghaus, P, Boersma, D J, Braun, J, Chirkin, D, Desiati, P, Diaz-Velez, J C, Dumm, J P, Eisch, J, Finley, C, Ganugapati, R, Gladstone, L, Grullon, S, Halzen, F, Hanson, K, Hill, G C, Hoshina, K, & Jacobsen, J. Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II. United States. https://doi.org/10.1103/PHYSREVD.79.102005
Abbasi, R, Andeen, K, Baker, M, Berghaus, P, Boersma, D J, Braun, J, Chirkin, D, Desiati, P, Diaz-Velez, J C, Dumm, J P, Eisch, J, Finley, C, Ganugapati, R, Gladstone, L, Grullon, S, Halzen, F, Hanson, K, Hill, G C, Hoshina, K, and Jacobsen, J. 2009. "Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II". United States. https://doi.org/10.1103/PHYSREVD.79.102005.
@article{osti_21296296,
title = {Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II},
author = {Abbasi, R and Andeen, K and Baker, M and Berghaus, P and Boersma, D J and Braun, J and Chirkin, D and Desiati, P and Diaz-Velez, J C and Dumm, J P and Eisch, J and Finley, C and Ganugapati, R and Gladstone, L and Grullon, S and Halzen, F and Hanson, K and Hill, G C and Hoshina, K and Jacobsen, J},
abstractNote = {The AMANDA-II detector, operating since 2000 in the deep ice at the geographic South Pole, has accumulated a large sample of atmospheric muon neutrinos in the 100 GeV to 10 TeV energy range. The zenith angle and energy distribution of these events can be used to search for various phenomenological signatures of quantum gravity in the neutrino sector, such as violation of Lorentz invariance or quantum decoherence. Analyzing a set of 5511 candidate neutrino events collected during 1387 days of livetime from 2000 to 2006, we find no evidence for such effects and set upper limits on violation of Lorentz invariance and quantum decoherence parameters using a maximum likelihood method. Given the absence of evidence for new flavor-changing physics, we use the same methodology to determine the conventional atmospheric muon neutrino flux above 100 GeV.},
doi = {10.1103/PHYSREVD.79.102005},
url = {https://www.osti.gov/biblio/21296296}, journal = {Physical Review. D, Particles Fields},
issn = {0556-2821},
number = 10,
volume = 79,
place = {United States},
year = {Fri May 15 00:00:00 EDT 2009},
month = {Fri May 15 00:00:00 EDT 2009}
}