NEVOD-DECOR experiment: Results and future. Journal of Physics: Conference Series Volume 409, Issue 1, 2013, Article number 012009

14 сентября 2018
239
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Контактные данные автора публикации Saavedra, O.a , Amelchakov, M.B.b, Barbashina, N.S.b, Bogdanov, A.G.b, Chernov, D.V.b, Chiavassa, A.a, Dushkin, L.I.b, Khokhlov, S.S.b, Khomyakov, V.A.b, Kindin, V.V.b, Kokoulin, R.P.b , Kompaniets, K.G.b, Mannocchi, G.
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Аннотация

Russian-Italian NEVOD-DECOR experiment on the measurements of the local muon density spectra (LMDS) at various zenith angles gave possibility to obtain information on primary cosmic ray flux and interaction characteristics in a record wide energy range from 1015 to more than 1018 eV. Comparison of the measurement results with CORSIKA-based simulations showed the increase of LMDS slope at PeV energies of primaries (corresponding to the first knee); a trend to a heavier primary mass composition above the knee; indication for a second knee (a further increase of the spectrum slope near 1017 eV). At large zenith angles and high muon densities (corresponding to primary energies around 1018 eV) a considerable excess of muon bundle events in comparison with the expectation based on independent estimates of the primary spectrum and widely used hadron interaction models has been found. In 2011, a new phase of measurements of the energy spectrum of cascade showers initiated by high-energy muons in water and of the energy deposit of muon bundles at various zenith angles and muon multiplicities started. Further plans include the deployment of a traditional EAS array around the NEVOD-DECOR complex.



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Indexed keywords

Cosmic ray flux; Energy deposits; Energy spectra; High energy; Interaction characteristics; Interaction model; Measurement results; Measurements of; Primary energies; Primary mass; Primary spectra; Wide energy range; Zenith angle
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