2009/02/04 by D. Ardouin, Daniel Ardouin, Didier Charrier +7 · 7 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Cosmic Phenomena #COSMIC cancer database #Computer science #Cosmic ray #Dark Matter and Cosmic Phenomena #Neutrino #Neutrino Physics Research #Noise (video) #Particle physics #Physics #astro-ph.HE #astro-ph.IM
paper · pdf · doi:10.1016/j.nima.2009.03.041
published in Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 604(1-2), S85-S87 (Elsevier BV) · 4pages, 3 figures, Contribution to appear in the proceedings of ARENA 2008 conference
arxiv created 2009/02/04 · openalex publication_date 2009/03/20 · arxiv updated 2010/04/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The recent demonstration by the CODALEMA Collaboration of the ability of the radio-detection technique for the characterization of UHE cosmic-rays calls for the use of this powerful method for the observation of UHE neutrinos. For this purpose, an adaptation of the existing 21CM Array (China) is presently under achievment. In an exceptionally low electromagnetic noise level, 10160 log-periodic 50-200 MHz antennas sit along two high valleys, surrounded by mountain chains. This lay-out results in 30-60 km effective rock thicnesses for neutrino interactions with low incidence trajectories along the direction of two 4-6 km baselines. We will present first in-situ radio measurements demonstrating that this environment shows particularly favourable conditions for the observation of electromagnetic decay signals of taus originating from the interaction of 1017-20 eV tau neutrinos.