Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9827440 | Astroparticle Physics | 2005 | 15 Pages |
Abstract
Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 1016 eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following Eâ2, with an equal mix of all flavors, is limited to E2Φ(1015 eV < E < 3 Ã 1018 eV) ⩽ 0.99 Ã 10â6 GeV cmâ2 sâ1 srâ1 at 90% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bounds to specific extraterrestrial neutrino flux predictions are also presented.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
M. Ackermann, J. Ahrens, H. Albrecht, D. Atlee, X. Bai, R. Bay, M. Bartelt, S.W. Barwick, T. Becka, K.H. Becker, J.K. Becker, E. Bernardini, D. Bertrand, D.J. Boersma, S. Böser, O. Botner, A. Bouchta, O. Bouhali, G. Yodh,