Cosmic rays: extragalactic and Galactic
Ya. N. Istomin

TL;DR
This paper analyzes high-energy cosmic ray fluxes, suggesting a power-law distribution for extragalactic rays similar to Galactic ones, and proposes that Galactic cosmic rays originate from past jet activity at the Galactic center, explaining the knee in the spectrum.
Contribution
It introduces a model linking Galactic and extragalactic cosmic rays, estimating source densities, and explaining the spectral knee through particle escape and diffusion effects.
Findings
Extragalactic cosmic ray power density follows a E^{-2.7} distribution.
Galactic cosmic rays likely originated from past jet activity in the Galactic center.
The spectral knee is explained by energy-dependent particle escape from the Galaxy.
Abstract
From the analysis of the flux of high energy particles, , it is shown that the distribution of the power density of extragalactic rays over energy is of the power law, , with the same index of that has the distribution of Galactic cosmic rays before so called 'knee', . However, the average power of extragalactic sources, which is of , at least two orders exceeds the power emitted by the Galaxy in cosmic rays, assuming that the density of galaxies is estimated as . Considering that such power can be provided by relativistic jets from active galactic nuclei with the power , we estimate the density of extragalactic sources of cosmic rays as . Assuming the same nature of…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Radio Astronomy Observations and Technology
