Propagation of extragalactic high energy cosmic and {gamma} rays

Journal Article · Sat Aug 01 04:00:00 EDT 1998 · Physical Review, D

DOI:https://doi.org/10.1103/PhysRevD.58.043004· OSTI ID:639847

Lee, S ^[1]

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1. Department of Physics, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637-1433 (United States)

The observation of air showers from elementary particles with energies exceeding 10{sup 20}thinspeV poses a puzzle to the physics and astrophysics of cosmic rays which is still unresolved. Explaining the origin and nature of these particles is a challenge. In order to constrain production mechanisms and sites, one has to account for the processing of particle spectra by interactions with radiation backgrounds and magnetic fields on the way to the observer. In this paper, I report on an extensive study on the propagation of extragalactic nucleons, {gamma}-rays, and electrons in the energy range between 10{sup 8}thinspeV and 10{sup 25}thinspeV. We have devised an efficient numerical method to solve the transport equations for cosmic ray spectral evolution. The universal radiation background spectrum in the energy range between {approx_equal}10{sup {minus}9}thinspeV and {approx_equal}10thinspeV is considered in the numerical code, including the diffuse radio background, the cosmic microwave background, and the infrared-optical background, as well as a possible extragalactic magnetic field. We apply the code to compute the particle spectra predicted by several models of ultrahigh energy cosmic ray origin. A comparison with the observed fluxes, especially the diffuse {gamma}-ray background in several energy ranges, allows one to constrain certain classes of models. {copyright} {ital 1998} {ital The American Physical Society}

• OSTI ID: 639847
• Journal Information: Physical Review, D, Journal Name: Physical Review, D Journal Issue: 4 Vol. 58; ISSN PRVDAQ; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
BACKGROUND RADIATION
COSMIC RAY PROPAGATION
DIFFUSION
ENERGY SPECTRA
EXTENSIVE AIR SHOWERS
GALAXIES
GAMMA RADIATION
INTERSTELLAR MAGNETIC FIELDS
MICROWAVE RADIATION