Turbulence and turbulent mixing in natural fluids
Carl H. Gibson (Univ. Cal. San Diego)

TL;DR
This paper proposes that turbulence from the big bang influences cosmic structures, suggesting turbulence fossils are observable in the universe's large-scale formations and cosmic microwave background anisotropies.
Contribution
It introduces a novel theory linking big bang turbulence to cosmic structure formation and fossil turbulence observations in the universe.
Findings
Cosmic microwave background anisotropies show turbulence fossils.
Large-scale cosmic structures align with turbulence fossil predictions.
Proto-galaxies and dark matter are linked to turbulence-driven fragmentation.
Abstract
Turbulence and turbulent mixing in natural fluids begins with big bang turbulence powered by spinning combustible combinations of Planck particles and Planck antiparticles. Particle prograde accretions on a spinning pair releases 42% of the particle rest mass energy to produce more fuel for turbulent combustion. Negative viscous stresses and negative turbulence stresses work against gravity, extracting mass-energy and space-time from the vacuum. Turbulence mixes cooling temperatures until strong-force viscous stresses freeze out turbulent mixing patterns as the first fossil turbulence. Cosmic microwave background temperature anisotropies show big bang turbulence fossils along with fossils of weak plasma turbulence triggered as plasma photon-viscous forces permit gravitational fragmentation on supercluster to galaxy mass scales. Turbulent morphologies and viscous-turbulent lengths appear…
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