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The cosmic web and microwave background fossilize the first turbulent combustion

Published online by Cambridge University Press:  12 October 2016

Carl H. Gibson  and
R. Norris Keeler
Carl H. Gibson
Affiliation:
MAE and SIO, Univ. of Cal. San Diego, La Jolla, CA, 92093-0411, USA email: cgibson@ucsd.edu
R. Norris Keeler
Affiliation:
6652 Hampton Park Court, McLean VA 22101, USA email: rnkeeler@verizon.net
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Abstract

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Collisional fluid mechanics theory predicts a turbulent hot big bang at Planck conditions from large, negative, turbulence stresses below the Fortov-Kerr limit (< −10113Pa). Big bang turbulence fossilized when quarks formed, extracting the mass energy of the universe by extreme negative viscous stresses of inflation, expanding to length scales larger than the horizon scale ct. Viscous-gravitational structure formation by fragmentation was triggered at big bang fossil vorticity turbulence vortex lines during the plasma epoch, as observed by the Planck space telescope. A cosmic web of protogalaxies, protogalaxyclusters, and protogalaxysuperclusters that formed in turbulent boundary layers of the spinning voids are hereby identified as expanding turbulence fossils that falsify CDMHC cosmology.

Keywords

turbulencecosmologydark matterdark energy
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S308: The Zeldovich Universe: Genesis and Growth of the Cosmic Web , June 2014 , pp. 636 - 637
Copyright
Copyright © International Astronomical Union 2016 

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