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Flux limits on ultra high energy neutrinos with AMANDA-B10
Astroparticle Physics 22(339-353): 2005
Handle: Document-17259
Owner: Site Administrator (User-2, admin:DocuShare)DS
Friday, October 14, 2005 02:45:01 PM CDT
Tuesday, April 3, 2007 05:49:15 PM CDT
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  • The experimental data sample is reduced to 263,000 events, or 6.5% of the initial sample.
  • Using data from the combined SPASE-AMANDA experiment, a similar trend to heavier primaries at higher energies is seen [29].
  • To investigate the sensitivity of the analysis to the composition of the primary cosmic rays, the proton and iron content was varied between 0% and 100%.
  • Allowing a minimum of 20% of protons or iron as extremes decreases the uncertainty to about 15%, the value used in this analysis.
  • The variation of the optical properties leads to the largest error of 34%, the absolute sensitivity of the OM contributes 15%, the neutrino cross section 8% and the muon propagation 6%.
  • 1sr?1. ...
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