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
- DOI
- 10.1063/1.2077201;
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)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37031634
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCELERATION; BLACK HOLES; COSMIC GAMMA BURSTS; COSMIC RAY SOURCES; GALAXIES; HOT SPOTS; LORENTZ INVARIANCE; NEUTRONS; PROTONS; SUPERGIANT STARS; SUPERNOVAE; WOLF-RAYET STARS
- Descriptors DEC
- BARYONS; BINARY STARS; COSMIC RADIATION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; GIANT STARS; HADRONS; INVARIANCE PRINCIPLES; IONIZING RADIATIONS; MAIN SEQUENCE STARS; NUCLEONS; PRIMARY COSMIC RADIATION; RADIATIONS; STARS; VARIABLE STARS
Optional Information
- Notes
- (c) 2005 American Institute of Physics