• Corpus ID: 15944270

Radio limits on an isotropic flux of >100 EeV cosmic neutrinos

  title={Radio limits on an isotropic flux of >100 EeV cosmic neutrinos},
  author={P. W. Gorham and Kurt M. Liewer and Charles J. Naudet and D. Williams},
  journal={arXiv: Astrophysics},
We report on results from about 30 hours of livetime with the Goldstone Lunar Ultra-high energy neutrino Experiment (GLUE). The experiment searches for ≤ 10 ns microwave pulses from the lunar regolith, appearing in coincidence at two large radio telescopes separated by about 22 km and linked by optical fiber. The pulses can arise from subsurface electromagnetic cascades induced by interactions of up-coming ∼ 100 EeV neutrinos in the lunar regolith. A new triggering method implemented after the… 

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  • Ap.J
  • 2000
Phys Rev. E
  • Phys Rev. E
  • 2000
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  • 1996
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  • Zeit. Phys
  • 1966