Turbulence, turbulent mixing, and gravitational structure formation in the early Universe

Carl H. Gibson

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arXiv · astro-ph/0110248

Turbulence, turbulent mixing, and gravitational structure formation in the early Universe

Carl H. Gibson

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Abstract

Turbulence and turbulent mixing of temperature powered the big bang formation of the universe at Planck length, time, and temperature scales. Planck-Kerr inertial-vortex forces balanced Planck gravitational forces to produce Planck (particle-pair) gas, Planck-gas turbulence and space-time-energy. Inflation at the strong force temperature fossilized the turbulence. Gluon-neutrino-photon bulk viscous forces exceeded gravitational and inertial-vortex forces of the baryonic (ordinary) matter during the radiation dominated hot plasma epoch, and large diffusive velocities of the weakly interacting nonbaryonic dark matter (possibly neutrinos) prevented gravitational structure formation of this material, contrary to the 1902 Jeans acoustic criterion and "cold dark matter" models. The first plasma structures were proto-galaxy-super-cluster fragments and voids triggered by turbulent-viscous-gravitational masses matching the horizon mass at time 10^12 s. The last plasma structures formed were proto-galaxies. At the 10^13 s plasma-gas transition, the proto-galaxies fragmented to form proto-globular-star-cluster clumps of earth-mass primordial-fog-particles (PFPs) that now comprise the baryonic dark matter. Observational evidence of PFPs is provided by young globular star clusters formed when galaxies merge, thousands of cometary knots seen around dying stars, and the rapid twinkling of lensed quasar images.

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Carl H. Gibson. 2001-10-12. Turbulence, turbulent mixing, and gravitational structure formation in the early Universe. https://arxiv.org/abs/astro-ph/0110248

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