Published October 2006 | Version v1
Journal article

Galactic cosmic rays

  • 1. Max-Planck Institute for Radioastronomy and Department of Physics and Astronomy, University of Bonn, Bonn (Germany)

Description

In this brief review we describe the theory of the origin of Galactic cosmic rays. The concept that interaction near the source is the dominant source of γ-rays, and spallation secondaries seems best suited to explain the EGRET γ-spectrum of the inner Galaxy, the abundances of light elements, the anti-protons and the positrons. Also the chemical abundances seem best described as resulting from the chemical composition of massive star winds. This leads to a supernova mechanism, long known, that the magneto-rotational mechanism provides the energy, about 1052 erg, for the explosion of the most massive stars; this mechanism naturally allows to understand jet-supernovae and Gamma Ray Bursts from its underlying symmetry. A key theoretical question remains open: the role of magnetic fields, both in the transport of cosmic rays in the Galaxy, as well as in the enhancement they may get in shock waves on various length scales, either starting with existing magnetic fields, or starting from electric current systems. An ultimate hope and expectation obviously is, once we understand the origin and physics of cosmic rays, to turn them into a tool to understand to understand the nature of matter at a yet deeper level

Availability note (English)

Available online at http://stacks.iop.org/1742-6596/47/78/jpconf6_47_009.pdf or at the Web site for the Journal of Physics. Conference Series (Online) (ISSN 1742-6596) http://www.iop.org/

Additional details

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
47
Journal Issue
1
Journal Page Range
p. 78-85
ISSN
1742-6596

Conference

Title
Workshop on physics at the end of the galactic cosmic ray spectrum
Dates
26-30 Apr 2005
Place
Aspen, CO (United States)