Published September 28, 2005 | Version v1
Journal article

Particle Acceleration: From Galaxies to Large Scale Structure

  • 1. Dept. of Astronomy, Indiana University, Bloomington, IN (United States)
  • 2. Department of Physics and Astronomy, University of Bonn (Germany)
  • 3. Max-Planck Institute for Radioastronomy, Auf dem Huegel 69, D-53121 Bonn (Germany)
  • 4. Space Research Institute, Profsoyuznaya Str. 84/32, Moscow 117997 (Russian Federation)

Description

In this brief review we discuss current efforts to understand the origin of energetic particles, focussing here on the recent work on the physics of supernova explosions. Acceleration to the highest energy may come from jets and hot spots emanating from massive black holes. If the sky remains smooth in the arrival directions of ultrahigh energy cosmic rays to the highest energies, then we need new sources, and one extreme speculation would be to invoke Lorentz Invariance Violation, with proton decay, neutron survival, and no strong photomeson interaction to higher energy. For the Galactic cosmic rays explosions of red supergiant stars and Wolf Rayet stars may provide much of the cosmic rays. This is intimately connected with the physics of their explosion, and implies that the magneto-rotational mechanism is the main one chosen by Nature. This offers a consistent picture for the X-ray fans of Cas A, and gamma ray bursts. Each of these concepts leads to clear predictions. It will be quite an achievement to prove this or any other proposal -- none is without difficulties. We do have potentially a full theory to account for cosmic rays at all energies; crucial tests will be performed with the current new instruments

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
784
Journal Issue
1
Journal Page Range
p. 385-395
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
From laboratory and stars to primordial structures
Acronym
International conference on magnetic fields in the universe
Dates
28 Nov - 3 Dec 2004
Place
Angra dos Reis (Brazil)

Optional Information

Notes
(c) 2005 American Institute of Physics