arXiv subjects

T. T. Barnaveli Jr

Publications and source records attributed to T. T. Barnaveli Jr.

3 recordsLinked to original sources

arXiv2016

About the possible signature of pion bose condensation contribution in the high energy cosmic ray nuclear interactions

The events of anomalous energy deposit and high number of hadrons in hadron calorimeter, often not accompanied at all, or accompanied by very small EAS of cosmic rays, are observed by means of the complex installation aimed at research of cosmic rays. The data quoted and their analysis point to the real contribution and the essential role of pion Bose condensation in high energy nuclear interactions. The possibility of the existence of such process in the nuclear matter (in the neutron stars and in some kinds of the nuclei) was proposed by A.B.Migdal in 1971.

astro-ph.HE↗

arXiv2006

On some peculiarities of cosmic gamma-radiation in the energy range ~ 10^14 - 10^15 eV

The distribution of EAS hadronic component energy fluxes through the ionization calorimeter in the primary energy range ~ 3x10^13 - 10^16 eV is considered. The EAS, carrying the zero or the minimal flux of the hadron component energy are extracted. The conclusion supports the existence of izotropic gamma-radiation in the primary energy region E_0 ~ 1x10^14 - 2x10^15 eV. This radiation has a spectrum of a form, close to the bell-like one, with the maximum at E_0 ~ 2.2x10^14 ev and with an additional local maximum at E_0 ~ 1.6x10^15 eV.

astro-ph↗

arXiv2003

Change of Primary Cosmic Radiation Nuclear Conposition in the Energy Range $10^{15} - 10^{17}$ eV as a Result of the Interaction with the Interstellar Cold Background of Light Particles

In this paper the updated arguments in favor of a simple model, explaining from the united positions all peculiarities of the Extensive Air Shower (EAS) hadron E_h(E_0) (and muon E_mu(E_0)) component energy fluxes dependence on the primary particle energy E_0 in the primary energy region 10^{15} - 10^{17} eV are represented. These peculiarities have shapes of consequent distinct deeps of a widths dE_h/E_h of the order of 0.2 and of relative amplitudes dL/L of the order of {0.1 - 1.0}, and are difficult to be explained via known astrophysical mechanisms of particle generation and acceleration. In the basis of the model lies the destruction of the Primary Cosmic Radiation (PCR) nuclei on some monochromatic background of interstellar space, consisting of the light particles of the mass in the area of 36 eV (maybe the component of a dark matter). The destruction thresholds of PCR different nuclear components correspond to the peculiarities of E_h(E_0). In this work the results of the recent treatment of large statistical material are analyzed. The experimental results are in good agreement with the Monte-Carlo calculations carried out in the frames of the proposed model.

astro-ph↗