The baryon-symmetric domain cosmology and the cosmic X-ray background

Details The baryon-symmetric domain cosmology and the cosmic X-ray background The baryon-symmetric domain cosmology and the cosmic X-ray background

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.135..291y&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 135, no. 2, July 1987, p. 291-300.

Astronomy and Astrophysics

Astrophysics

1

Baryons, Cosmic X Rays, Cosmology, Galactic Nuclei, Astronomical Models, Grand Unified Theory

Scientific paper

The baryon-symmetric domain cosmology (BSDC) of Stecker et al. (1971) have explained the diffuse gamma-ray background. However, evidence has shown that AGNs are likely contributors to the diffuse gamma-ray background, so there are some problems with the original formulations. The original formulations are reviewed, and the expressions are modified for the matter temperature and the redshifts at which the cosmic radiation from the BSDC becomes significantly absorbed. In this way, it is shown that the cosmic radiation from the BSDC agrees remarkably with the cosmic X-ray background from about 1 keV to about 100 keV.

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