24-26 June 2025
National Research Nuclear University MEPhI
Europe/Moscow timezone

Investigations of extensive air showers in the Experimental complex NEVOD

Not scheduled
15m
National Research Nuclear University MEPhI

National Research Nuclear University MEPhI

Kashirskoe shosse 31, Moscow, Russian Federation, 115409
Original Talk Cosmic rays (nuclei, gammas, neutrinos) of very high energies (> 100 TeV) Cosmic rays (nuclei, gammas, neutrinos) of very high energies (> 100 TeV)

Speaker

Elena Yuzhakova (MEPhI)

Description

The main information about high-energy cosmic rays (above 10^15 eV) is provided by the extensive air showers (EAS), which are formed as a result of interaction of primary cosmic rays (PCR) with nuclei of atmospheric atoms. In the energy range from 10^15 to 10^17 eV, the PCR energy spectrum reconstructed by the data of EAS experiments has features which cannot be explained within the frameworks of existing models of cosmic ray origin.

Studies of air-showers in the energy range of 10^15–10^17 eV are carried out in the Experimental complex NEVOD. The NEVOD-EAS array allows detection of the electron-photon component, the Calibration Telescope System ensures selection of the EAS muon component, and the URAN array measures the air-showers hadronic component.

The lateral distributions of the electron-photon, muon, and hadronic components of the air-showers obtained by the data from these facilities are presented. The technique for reconstructing EAS parameters and PCR energy spectrum based on the NEVOD-EAS array response is described.

Primary author

Co-authors

Mikhail Amelchakov (MEPhI) Aleksei Bogdanov (MEPhI) Andrea Chiavassa (Università di Torino) Semyon Khokhlov (National Research Nuclear University MEPhI) Evgeniy Khomchuk (MEPhi) Alena Konovalova (National Research Nuclear University MEPhI) Korneliia Nugaeva Ivan Shulzhenko (National Research Nuclear University MEPhI)

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