The NuMoon experiment: first results
S. Buitink, J. Bacelar, R. Braun, G. de Bruyn, H. Falcke, O. Scholten,, K. Singh, B. Stappers, R. Strom, R. al Yahyaoui

TL;DR
The NuMoon experiment searches for ultra high energy cosmic particles via radio pulses from the Moon, setting new limits on neutrino flux with initial data analysis from Westerbork Telescope.
Contribution
First analysis of NuMoon data demonstrating the potential to improve neutrino flux limits using lunar radio pulse detection.
Findings
Set a new upper limit on neutrino flux.
Analyzed 10 hours of observational data.
Demonstrated feasibility of lunar radio pulse detection for cosmic particles.
Abstract
The NuMoon project uses the Westerbork Synthesis Radio Telescope to search for short radio pulses from the Moon. These pulses are created when an ultra high energy cosmic ray or neutrino initiates a particle cascade inside the Moon's regolith. The cascade has a negative charge excess and moves faster than the local speed of light, which causes coherent Cherenkov radiation to be emitted. With 100 hours of data, a limit on the neutrino flux can be set that is an order of magnitude better than the current one (based on FORTE). We present an analysis of the first 10 hours of data.
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena · Particle Accelerators and Free-Electron Lasers
