Author/Authors :
Ackermann، نويسنده , , M. Bridget Ahrens، نويسنده , , J. and Albrecht، نويسنده , , H. and Atlee، نويسنده , , D. and Bai، نويسنده , , X. and Bay، نويسنده , , R. and Bartelt، نويسنده , , M. and Barwick، نويسنده , , S.W. and Becka، نويسنده , , T. and Becker، نويسنده , , K.H. and Becker، نويسنده , , J.K. and Bernardini، نويسنده , , E. and Bertrand، نويسنده , , D. and Boersma، نويسنده , , D.J. and B?ser، نويسنده , , S. and Botner، نويسنده , , O. and Bo، نويسنده ,
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 E−2, with an equal mix of all flavors, is limited to E2Φ(1015 eV < E < 3 × 1018 eV) ⩽ 0.99 × 10−6 GeV cm−2 s−1 sr−1 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.
Keywords :
Neutrino astronomy , UHE neutrinos , AMANDA , Neutrino telescopes
