Published June 1990 | Version v1
Journal article

On the origin of highest energy cosmic rays

  • 1. Tokyo Metropolitan Univ. (Japan). Dept. of Physics

Description

A possible mechanism of the acceleration of highest energy cosmic rays is proposed. Mildly relativistic shocks in radio galaxies, especially hot spots in radio lobes, are shown to be able to accelerate protons up to 1020 eV. To avoid energy losses through collisions with radio photons, the size and distance of the acceleration region from the nucleus must be larger than about 100 pc. Required cosmic ray luminosity for each radio galaxy is an order of 1041-42 erg·s-1, which is a modest fraction of the total luminosity. Anisotropy in the arrival direction should be observable towards nearby radio galaxies. (author)

Additional details

Publishing Information

Journal Title
Progress of Theoretical Physics (Kyoto)
Journal Volume
83
Journal Issue
6
Series
Prog. Theor. Phys. (Kyoto).
Journal Page Range
1071-1075
ISSN
0033-068X
CODEN
PTPKA

INIS

Country of Publication
Japan
Country of Input or Organization
Japan
INIS RN
21091720
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ACCELERATION; COSMIC RADIATION; ENERGY LOSSES; GALACTIC EVOLUTION; RADIO GALAXIES; RELATIVISTIC RANGE; SHOCK WAVES
Descriptors DEC
COSMIC RADIO SOURCES; ENERGY RANGE; GALAXIES; IONIZING RADIATIONS; RADIATIONS