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Journal ArticleDOI

Cosmic ray propagation in a closed galaxy

TLDR
In this article, a simple model of cosmic ray propagation is proposed from which the major experimental results can be derived: the model reproduces the observed nuclear abundances and accounts for the observed changes of nuclear composition with energy.
Abstract
A simple model of cosmic ray propagation is proposed from which the major experimental results can be derived: The model reproduces the observed nuclear abundances and accounts for the observed changes of nuclear composition with energy, the high degree of isotropy of cosmic ray flux at all energies, and the high degree of its constancy throughout the history of the Solar System. It is consistent with the observed size distribution of extensive airshowers, the intensity and energy distribution of the electron component, and the diffuse emission of γ-rays and radio waves. The model is characterized by the two basic assumptions: (1) that cosmic rays have been injected at an unchanging rate by sources located in the galactic spiral arms and (2) that a large-scale magnetic field retains all particles in our galaxy, where they interact with interstellar gas, so that all complex nuclei are finally fragmented and their energy dissipated in meson production and electro-magnetic interactions.

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Citations
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Cosmic rays and particle physics.

TL;DR: In this paper, the authors present a model for accelerating a particle to >100 TeV using cosmic rays and neutrino-induced muons, which they call cosmic ray showers.
Journal ArticleDOI

Spallation processes and nuclear interaction products of cosmic rays

TL;DR: The effects of nuclear spallation, production of radioactive nuclides and the time dependence of their decay provide valuable information on the acceleration and propagation of cosmic rays, their nuclear transformations, and their confinement time in the Galaxy.
Journal ArticleDOI

Calculation of the equilibrium antiproton spectrum

TL;DR: A thorough discussion of the equilibrium antiproton spectrum prediction for the usual leaky-box model, the closed-galaxy model of Rasmussen and Peters (1975), and the revised closed-gasea model of Peters and Westergaard (1976) is presented in this article.
Journal ArticleDOI

Antiprotons in the cosmic radiation

TL;DR: In this article, an improved calculation of the energy spectrum of p expected for the standard leaky box model was presented, and it was shown that even the enhanced secondary p production in the closed Galaxy model of Peters and Westergaard9 fails by a wide margin to reproduce the high observed flux at low energies.
Journal ArticleDOI

The role of antiprotons in cosmic-ray physics

TL;DR: In this article, the energy spectrum of cosmic-ray antiprotons has been studied, from about 200 MeV to about 15 GeV, and it is shown that no single model could predict correctly the observed energy spectrum over the entire energy region.
References
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Journal ArticleDOI

Origin of cosmic rays.

TL;DR: In this paper, it was claimed that the observed isotropy of the cosmic rays incident on the earth is simply a consequence of a magnetic field assumed to exist in interstellar space, and the basis for this claim is that a single particle of energy n and charge e is deflected through an appreciable angle after travelling a distance d across a magnetic magnetic field of intensity H, provided n equal to 1010 eV., e equal to the electronic charge (4·77 × 10-10 E.G.U.), and d equal to radius of the galaxy (∽3
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High energy gamma ray results from the second small astronomy satellite

TL;DR: A high energy (35 MeV) gamma ray telescope employing a thirty-two level magnetic core spark chamber system was flown on SAS 2 as mentioned in this paper, and the high energy galactic gamma radiation was observed to dominate over the general diffuse radiation along the entire galactic plane, and when examined in detail, the longitudinal and latitudinal distribution seem generally correlated with galactic structural features.
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Charge composition and energy spectra of cosmic-ray nuclei at energies above 20 GeV per nucleon

TL;DR: In this paper, les abondances relatives des elements de charge 4 ≤ Z ≤ 28 and le spectre d'energie absolu de ces elements sont determined.
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