On radio detection of ultra-high energy neutrinos in Antarctic ice
Interactions of ultrahigh energy neutrinos of cosmological origin in large volumes of dense, radio-transparent media can be detected via coherent Cherenkov emission from accompanying electromagnetic showers. Antarctic ice meets the requirements for an efficient detection medium for a radio frequency...
| Main Authors: | , , |
|---|---|
| Language: | English |
| Published: |
1996
|
| Subjects: | |
| Online Access: | http://cds.cern.ch/record/285136 |
| Summary: | Interactions of ultrahigh energy neutrinos of cosmological origin in large volumes of dense, radio-transparent media can be detected via coherent Cherenkov emission from accompanying electromagnetic showers. Antarctic ice meets the requirements for an efficient detection medium for a radio frequency neutrino telescope. We carefully estimate the sensitivity of realistic antennas embedded deep in the ice to 100 MHz - 1 GHz signals generated by predicted neutrino fluxes from active galactic nuclei. Our main conclusion is that a {\it single radio receiver} can probe a \sim 1 {\rm km}^3 volume for events with primary energy near 2 PeV and that the total number of events registered would be roughly 200 to 400 {\rm year}^{-1} in our most conservative estimate. An array of such receivers would increase sensitivity dramatically. A radio neutrino telescope could directly observe and test our understanding of the most powerful particle accelerators in the universe, simultaneously testing the standard theory of particle physics at unprecedented energies. |
|---|