Skip to main content
Article thumbnail
Location of Repository

Search for ultra high-energy neutrinos with AMANDA-II

By M. Ackermann, G. de Vries-Uiterweerd, M.R. Duvoort, J. Heise and N.J.A.M. van Eijndhoven

Abstract

A search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data recorded between 2000 and 2002. Above 107 GeV, the Earth is essentially opaque to neutrinos. This fact, combined with the limited overburden of the AMANDA-II detector (roughly 1.5 km), concentrates these ultra high-energy neutrinos at the horizon. The primary background for this analysis is bundles of downgoing, high-energy muons from the interaction of cosmic rays in the atmosphere. No statistically significant excess above the expected background is seen in the data, and an upper limit is set on the diffuse all-flavor neutrino flux of E2 90%CL <2.7 × 10−7 GeV cm−2 s−1 sr−1 valid over the energy range of 2 × 105 GeV to 109 GeV. A number of models which predict neutrino fluxes from active galactic nuclei are excluded at the 90% confidence level

Year: 2008
OAI identifier: oai:dspace.library.uu.nl:1874/32656
Download PDF:
Sorry, we are unable to provide the full text but you may find it at the following location(s):
  • http://dspace.library.uu.nl:80... (external link)
  • Suggested articles


    To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request.