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Investigation of primary cosmic rays at the Moon’s surface |
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| Authors: | N N Kalmykov A A Konstantinov R A Muhamedshin D M Podorozhniy L G Sveshnikova A N Turundaevskiy L G Tkachev A P Chubenko O A Vasilyev |
| Institution: | 1. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119992, Russia 2. Institute for Nuclear Research, Russian Academy of Sciences, pr. Shestidesyatiletiya Oktyabrya 7a, Moscow, 117312, Russia 3. Joint Institute for Nuclear Research, Dubna, Moscow oblast, 141980, Russia 4. Lebedev Institute of Physics, Russian Academy of Sciences, Leninskii pr. 53, Moscow, 119991, Russia |
| Abstract: | The possibility of experimentally studying primary cosmic rays at the Moon’s surface is considered. A mathematical simulations of showers initiated in the lunar regolith by high-energy particles of primary cosmic rays is performed. It is shown that such particles can in principle be recorded by simultaneously detecting three components of backscattered radiation (secondary neutrons, gamma rays, and radio emission). |
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