Cold dark matter cosmology conflicts with fluid mechanics and observations

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dc.creatorGibson, Carl H.
dc.date2006-06-04
dc.date2006-10-23
dc.date.accessioned2026-07-07T11:25:39Z
dc.date.available2026-07-07T11:25:39Z
dc.descriptionCold 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 (10^46 kg), cluster, and galaxy-mass (10^42 kg) clouds in the primordial plasma with the large fossil density turbulence (rho_o ~ 3x10-17 kg m-3) of the first fragmentation at 10^12 s, and a protogalaxy linear and spiral clump morphology reflecting maximum stretching near vortex lines of the plasma turbulence at the 10^13 s plasma-gas transition. Gas protogalaxies fragmented into proto-globular-star-cluster mass (10^36 kg) clumps of protoplanet gas clouds that are now frozen as earth-mass (10^24-^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 10^16 s, but support the immediate gentle formation of small Population II first stars at 10^13 s in globular-star-clusters from HGD.
dc.description7 pages, 5 figures, J. Applied Fluid Mech. format
dc.identifierhttps://arxiv.org/abs/astro-ph/0606073
dc.identifierhttp://arxiv.org/abs/astro-ph/0606073
dc.identifierJ.Appl.FluidMech.2:1-8,2008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195573
dc.subjectAstrophysics
dc.titleCold dark matter cosmology conflicts with fluid mechanics and observations
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