Abstract
An estimate of the feasibility of the ultrahigh-energy cosmic ray and neutrino detection using a lunar satellite-borne radio receiver is presented. The data obtained in the proposed experiment will make resolving the current contradictions in the ultrahigh-energy cosmic ray spectra measured with the major ground-based instruments possible. Moreover, they will enable us to considerably extend the accessible energy range and to check predictions of various models of the origin of the highest-energy particles in the Universe. At the same time the lunar radio detector provides a means of searching for ultrahigh-energy neutrinos with a high sensitivity combined with a very large target effective mass.
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Original Russian Text © G.A. Gusev, B.N. Lomonosov, K.M. Pichkhadze, N.G. Polukhina, V.A. Ryabov, T. Saito, V.K. Sysoev, E.L. Feinberg, V.A. Tsarev, V.A. Chechin, 2006, published in Kosmicheskie Issledovaniya, 2006, Vol. 44, No. 1, pp. 22–42.
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Gusev, G.A., Lomonosov, B.N., Pichkhadze, K.M. et al. Detection of ultrahigh-energy cosmic rays and neutrinos by radio method using artificial lunar satellites. Cosmic Res 44, 19–38 (2006). https://doi.org/10.1134/S0010952506010035
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DOI: https://doi.org/10.1134/S0010952506010035