Cold dark matter cosmology conflicts with fluid mechanics and observations
Abstract
Cold dark matter hierarchical clustering (CDMHC) cosmology based on the Jeans 1902 criterion for gravitational instability gives predictions about the early universe contrary to fluid mechanics and observations. Jeans neglected viscosity, diffusivity, and turbulence: factors that determine gravitational structure formation and contradict small structures (CDM halos) forming from non-baryonic dark matter particle candidates. From hydro-gravitational-dynamics (HGD) cosmology, viscous-gravitational fragmentation produced supercluster (1046 kg), cluster, and galaxy-mass (1042 kg) clouds in the primordial plasma with the large fossil density turbulence (rhoo ~ 3x10-17 kg m-3) of the first fragmentation at 1012 s, and a protogalaxy linear and spiral clump morphology reflecting maximum stretching near vortex lines of the plasma turbulence at the 1013 s plasma-gas transition. Gas protogalaxies fragmented into proto-globular-star-cluster mass (1036 kg) clumps of protoplanet gas clouds that are now frozen as earth-mass (1024-25 kg) Jovian planets of the baryonic dark matter, about 30,000,000 rogue planets per star. Observations contradict the CDMHCC prediction of large explosive Population III first stars at 1016 s, but support the immediate gentle formation of small Population II first stars at 1013 s in globular-star-clusters from HGD.
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