Authors: Sylwester Kornowski
The Planck CMB data lead to conclusion that there should be about two times more galaxy clusters than we observe. Here, applying the lacking part of ultimate theory, i.e. the Scale-Symmetric Theory, we show that the discrepancy follows from the collisions/mergers of protogalaxy clusters at the beginning of the expansion of the Universe. The time distance to most distant galaxies is 13.866 ± 0.096 Gyr but they are already 7.75 Gyr old so we cannot see the collisions of protogalaxy clusters. It is a wrong assumption that creation of galaxies can last a few hundred million years only. For 8 times more spiral galaxies than elliptical galaxies, we obtain that there should be observed about 1.8 times less galaxy clusters than it follows from the Planck CMB data.
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[v1] 2014-08-16 11:20:05 (removed)
[v2] 2015-03-03 03:38:56
[v3] 2016-01-05 14:39:29
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