Title of article
Limits on the ultra-high energy electron neutrino flux from the RICE experiment
Author/Authors
Kravchenko، نويسنده , , I. and Frichter، نويسنده , , G.M. and Miller، نويسنده , , T. and Piccirillo، نويسنده , , L. and Seckel، نويسنده , , D. and Spiczak، نويسنده , , G.M and Adams، نويسنده , , J. and Seunarine، نويسنده , , S. and Allen، نويسنده , , C. and Bean، نويسنده , , A. and Besson، نويسنده , , D. and Box، نويسنده , , D.J and Buniy، نويسنده , , R. and Drees، نويسنده , , J. and McKay، نويسنده , , D. and Meyers، نويسنده , , J. and Perry، نويسنده , , L. and Ralston، نويسنده , , J. and Razzaque، نويسنده , , S. and Schmitz، نويسنده , , D.W.، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2003
Pages
19
From page
195
To page
213
Abstract
Upper limits are presented on the diffuse flux of ultra-high energy νe, based on analysis of data taken by the RICE experiment during August, 2000. The RICE receiver array at South Pole monitors cold ice for radio-wavelength Cherenkov radiation resulting from neutrino induced in-ice showers. For energies above 1 EeV, RICE is an effective detector of over 15 km3 sr. Potential signal events are separated from backgrounds using vertex location, event reconstruction, and signal shape. These are the first terrestrial limits exploiting the physics of radio-Cherenkov emissions from charged current νe+N→e+N′ interactions.
Journal title
Astroparticle Physics
Serial Year
2003
Journal title
Astroparticle Physics
Record number
1329025
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