Published July 11, 2024 | Version v1
Journal article

Galactic origin of ultrahigh energy cosmic rays

  • 1. Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, 108840 Troitsk, Moscow, Russia
  • 2. Institute for Physical Science and Technology, University of Maryland, College Park, Maryland 20742, USA

Description

It is shown that the acceleration of particles by a powerful relativistic jet associated with the activity of a supermassive black hole in the Galactic Center several million years ago may explain the observed cosmic ray spectrum at energies higher than 1015eV. The accelerated particles are efficiently confined in the extended magnetized gas halo created by the supernova and central black hole activity just after the formation of the Galaxy. We found that both the heavy and light chemical composition of ultrahigh energy cosmic rays can be consistent with observations.

Additional details

Publishing Information

Journal Title
Physical Review D
Journal Volume
110
Journal Issue
2
Journal Page Range
11 pgs.
ISSN
1089-4918

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ACCELERATION; BLACK HOLES; COSMIC RADIATION; ENERGY SPECTRA; GALAXY NUCLEI; JETS; MILKY WAY; ORIGIN; SUPERNOVAE
Descriptors DEC
BINARY STARS; ERUPTIVE VARIABLE STARS; GALAXIES; IONIZING RADIATIONS; RADIATIONS; SPECTRA; STARS; VARIABLE STARS

Optional Information

Copyright
© 2024 American Physical Society
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