期刊
出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/j.nima.2009.03.037
关键词
Ultra-High Energy cosmic ray; UHE neutrinos; Radio waves
类别
资金
- STFC [ST/G002487/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/G002487/1] Funding Source: researchfish
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.
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