Abstract
We show that at wavelengths comparable to the length of the shower produced by an Ultra-High Energy cosmic ray or neutrino, radio signals are an extremely efficient way to detect these particles. First results are presented of an analysis of 20h of observation data for NuMoon project using the Westerbork Synthesis Radio Telescope to search for short radio pulses from the Moon. A limit on the neutrino flux is set that is a factor four better than the current one (based on FORTE satellite observations). (C) 2009 Elsevier B.V. All rights reserved.
| Original language | English |
|---|---|
| Pages (from-to) | S102-S105 |
| Number of pages | 4 |
| Journal | Nuclear instruments & methods in physics research section a-Accelerators spectrometers detectors and associated equipment |
| Volume | 604 |
| Issue number | 1-2 |
| DOIs | |
| Publication status | Published - 1-Jun-2009 |
| Event | 3rd International Workshop on Acoustic and Radio EeV Neutrino Detection Activities - , Italy Duration: 25-Jun-2007 → 27-Jun-2008 |
Keywords
- Ultra-High Energy cosmic ray
- UHE neutrinos
- Radio waves
- COHERENT RADIO EMISSION
- ENERGY COSMIC-RAYS
- NEUTRINOS
- SHOWERS
- PULSES