Radio Detection of UHE Cosmic Rays and Neutrinos off the Moon with Two 30 m Telescopes
Due to the Askaryan effect, radio emissions will be produced when ultra-high-energy (UHE) cosmic rays and neutrinos impact the lunar regolith. Many experiments have been proposed and performed to detect such radio emissions from the lunar regolith. However, none of the Cherenkov radio signals has be...
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Main Authors: | , , , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2024-12-01
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Series: | Universe |
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Online Access: | https://www.mdpi.com/2218-1997/11/1/7 |
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