Lunar radio Cherenkov observations of UHE neutrinos

Details Lunar radio Cherenkov observations of UHE neutrinos Lunar radio Cherenkov observations of UHE neutrinos

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nimpa.604s.106e&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 604, Issue 1-2, p. S106-S111.

Physics

4

Scientific paper

The lunar radio Cherenkov technique uses the moon as a large-volume detector for ultra-high energy (UHE) cosmic rays and neutrinos. We review the issues and techniques needed for sensitive radio detection of nanosecond pulses from UHE neutrino events in the lunar regolith. Historical experiments and limits are discussed. We compare experiments using single telescopes with focal plane array and both incoherent and coherent detection with aperture plane arrays of telescopes. Opportunities for future experiments at both high and low frequencies with massive arrays such as the SKA will be considered.

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