Abstract

The development of nuclear-electromagnetic cascade models in air in the late forties have shown informational content of the study of cores of extensive air showers (EAS). These investigations were the main goal in different experiments which were carried out over many years by a variety of methods. Outcomes of such investigations obtained in the HADRON experiment using an X-ray emulsion chamber (XREC) as a core detector are considered. The N e spectrum of EAS associated with γ-ray families, spectra of γ-rays (hadrons) in EAS cores and the N e dependence of the muon number, ⟨N μ ⟩, in EAS with γ-ray families are obtained for the first time at energies of 1015 –1017 eV with this method. A number of new effects were observed, namely, an abnormal scaling violation in hadron spectra which are fundamentally different from model predictions, an excess of muon number in EAS associated with γ-ray families, and the penetrating component in EAS cores. It is supposed that the abnormal behavior of γ-ray spectra and N e dependence of the muon number are explained by the emergence of a penetrating component in the 1st PCR spectrum ‘knee’ range. Nuclear and astrophysical explanations of the origin of the penetrating component are discussed. The necessity of considering the contribution of a single close cosmic-ray source to explain the PCR spectrum in the knee range is noted.

Highlights

  • The power spectrum of the primary cosmic radiation (PCR) has two specific ranges, namely, the so-called knee at energies of 1015–1018 eV and the range of energies higher than 1019 eV where cut off of the PCR spectrum is supposed

  • The main problem of these measurements is the timing of the X-ray emulsion chamber (XREC) data, that do not have a time reference, with data of the extensive air showers (EAS)-array electronic detectors

  • In accordance with nuclearelectromagnetic cascades (NEC) models, the main information on the type of the primary nucleus is concentrated in the spectra of the most energetic hadrons located in the central area of EAS (EAS core)

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Summary

Introduction

The power spectrum of the primary cosmic radiation (PCR) has two specific ranges, namely, the so-called knee at energies of 1015–1018 eV and the range of energies higher than 1019 eV where cut off of the PCR spectrum is supposed. The PCR energy spectrum has two rather sharp breaks in this range, namely, at energies of 3 and 70 PeV The origins of these peculiarities of the spectrum are still not clear though the main break at 3 PeV was found in 1958 [1]; evidence in favor of the second one was first observed in the nineties [2]. The main problem of these measurements is the timing of the XREC data, that do not have a time reference, with data of the EAS-array electronic detectors. The solution of this problem [4] has permitted to carry out such measurements in the HADRON experiment.

History
EAS experiment
Experiment Pamir
Experiment HADRON
Abnormal scaling violation in γ -rays spectra
Excess of muons in EAS with γ -ray families
The penetrating component
PCR spectrum and model of a close single source
Findings
Conclusions
Full Text
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