Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the Pierre Auger Observatory

Abstract

The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth’s crust. Tau leptons from ντ charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January 2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of ντ at EeV energies. Assuming an E⁻²ν differential energy spectrum the limit set at 90% C.L. is E2νdNντ/dEν<1.3×10⁻⁷  GeV cm⁻² s⁻¹ sr⁻¹ in the energy range 2×10¹⁷ eV<Eν<2×10¹⁹ eV.

Description
Keywords
COSMIC-RAYS, FLUORESCENCE DETECTOR, AIR-SHOWERS, SEARCH, EARTH, Physics, Multidisciplinary, Physics
Citation
Abraham, J., et al. (2008): Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory. Physical Review Letters, 100(21). DOI: http://dx.doi.org/10.1103/PhysRevLett.100.211101