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A&A 386, 1-11 (2002)
DOI: 10.1051/0004-6361:20020211
Implications of cosmological gamma-ray absorption
I. Evolution of the metagalactic radiation field
T. M. Kneiske1, K. Mannheim1 and D. H. Hartmann21 Universität Würzburg, Am Hubland, 97057 Würzburg, Germany
2 Clemson University, Clemson, SC 29634-0978, USA
(Received 9 July 2001 / Accepted 30 January 2002 )
Abstract
Gamma-ray absorption due to
-pair creation on cosmological scales
depends on the line-of-sight integral of the evolving density of low-energy photons
in the Universe, i.e. on the history of the diffuse, isotropic
radiation field.
Here we present and discuss a semi-empirical model for this metagalactic
radiation field based on stellar light produced and reprocessed in evolving galaxies.
With a minimum of parameters and assumptions,
the present-day background
intensity is obtained from the far-IR to the ultraviolet band.
Predicted model intensities are independent of cosmological parameters, since we require
that the comoving emissivity, as a function of redshift,
agrees with observed values obtained from deep galaxy surveys.
The far-infrared background at present predicted from optical galaxy surveys
falls short in explaining the observed one, and we show that this deficit can be removed
by taking into account (ultra)luminous infrared galaxies with a seperate star formation rate.
The accuracy and reliability of the model,
out to redshifts of
, allow a realistic estimate of the
attenuation length of GeV-to-TeV gamma-rays and its uncertainty, which will be
the focus of a subsequent paper.
Key words: galaxies: evolution -- ISM: general -- radiation mechanisms: general -- cosmology: observations
Offprint request: T. M. Kneiske, kneiske@astro.uni-wuerzburg.de
© ESO 2002
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