Difference between revisions of "Cosmic Matter and the Nonexpanding Universe"

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==Abstract==
 
==Abstract==
  
<em>Updated paper from: IEEE Transactions on Plasma Science, Vol. 17, No: 2 April 1989</em>. An increasingly large number of observations consistently reveal the existence of a much larger amount of intergalactic matter than presently accepted. Radio signals coming from directions between galaxies is discussed. An average density of matter in space of about 0.01 atom/cm3 is derived. It is known that the density of matter is compatible with many reliable observations. These results lead to a nonexpanding cosmological universe.[[Category:Scientific Paper]]
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<em>Updated paper from: IEEE Transactions on Plasma Science, Vol. 17, No: 2 April 1989</em>. An increasingly large number of observations consistently reveal the existence of a much larger amount of intergalactic matter than presently accepted. Radio signals coming from directions between galaxies is discussed. An average density of matter in space of about 0.01 atom/cm3 is derived. It is known that the density of matter is compatible with many reliable observations. These results lead to a nonexpanding cosmological universe.
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[[Category:Scientific Paper|cosmic matter nonexpanding universe]]
  
 
[[Category:Cosmology]]
 
[[Category:Cosmology]]

Revision as of 10:12, 1 January 2017

Scientific Paper
Title Cosmic Matter and the Nonexpanding Universe
Read in full Link to paper
Author(s) Grote Reber, Paul Marmet
Keywords {{{keywords}}}
Published 1989
Journal None
Volume 17
Number 2
No. of pages 10

Read the full paper here

Abstract

Updated paper from: IEEE Transactions on Plasma Science, Vol. 17, No: 2 April 1989. An increasingly large number of observations consistently reveal the existence of a much larger amount of intergalactic matter than presently accepted. Radio signals coming from directions between galaxies is discussed. An average density of matter in space of about 0.01 atom/cm3 is derived. It is known that the density of matter is compatible with many reliable observations. These results lead to a nonexpanding cosmological universe.