International audienceNeutrinos of astrophysical origin could be detected through the electromagnetic radiation of the particle showers induced in the atmosphere by their interaction in the Earth. This applies in particular for tau neutrinos of energies E > 10 16 eV following Earth-skimming trajectories. The ∼1° beaming of the radio emission in the forward direction however implies that the radio signal will likely fly above a detector deployed over a flat site and would therefore not be detected
Amplified Tau-airshower at horizons may well open a novel powerful windows, at PeV-EeV energy, to Ne...
High energy neutrinos can arise from a variety of processes. Interactions of ultra high energy cosmi...
Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse f...
International audienceNeutrinos of astrophysical origin could be detected through the electromagneti...
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the par...
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the par...
This paper investigates the potential to detect tau neutrinos in the energy range of 1–1000 PeV sear...
Cosmic neutrinos are expected to include a significant flux of tau neutrinos due to flavor mixing ov...
Cosmogenic neutrinos1 are expected from ultrahigh energy cosmic rays undergoing the GZK process2,3 a...
Ultra High Energy, UHE, Neutrino Astronomy should be soon tested looking toward the Earth. At presen...
International audienceCosmic neutrinos above a PeV are produced either within astrophysical sources ...
4pages, 3 figures, Contribution to appear in the proceedings of ARENA 2008 conferenceInternational a...
Amplified Tau-airshower at horizons may well open a novel powerful windows, at PeV-EeV energy, to Ne...
High energy neutrinos can arise from a variety of processes. Interactions of ultra high energy cosmi...
Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse f...
International audienceNeutrinos of astrophysical origin could be detected through the electromagneti...
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the par...
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the par...
This paper investigates the potential to detect tau neutrinos in the energy range of 1–1000 PeV sear...
Cosmic neutrinos are expected to include a significant flux of tau neutrinos due to flavor mixing ov...
Cosmogenic neutrinos1 are expected from ultrahigh energy cosmic rays undergoing the GZK process2,3 a...
Ultra High Energy, UHE, Neutrino Astronomy should be soon tested looking toward the Earth. At presen...
International audienceCosmic neutrinos above a PeV are produced either within astrophysical sources ...
4pages, 3 figures, Contribution to appear in the proceedings of ARENA 2008 conferenceInternational a...
Amplified Tau-airshower at horizons may well open a novel powerful windows, at PeV-EeV energy, to Ne...
High energy neutrinos can arise from a variety of processes. Interactions of ultra high energy cosmi...
Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse f...