Physics – Fluid Dynamics
Scientific paper
Nov 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..dfd.dn010g&link_type=abstract
American Physical Society, 53rd Annual Meeting of the Division of Fluid Dynamics November 19 - 21, 2000 Washington, DC Meeting I
Physics
Fluid Dynamics
Scientific paper
Recent high resolution cosmic microwave background (CMB) δ T/T maps show hot/cold spots that have been interpreted as acoustic, requiring powerful local sound sources. Alternatively, the spots may be non-acoustic fossils of buoyancy damped gravitational structure formation beginning in the plasma epoch about 30,000 years after the Big Bang, superimposed on fossil turbulent temperature fluctuations produced by the initial Big Bang singularity at Planck scales and then fossilized by inflation to scales larger than Batchelor or LH = ct scales, where c is the speed of light and t is the time, giving the observed k^1/3 spectrum rather than the hypothesized k^0 Harrison-Zel'dovich form. Gibson's (1996-2000) fluid mechanical theory of gravitational instability predicts viscous-gravitational supercluster formation in the hot plasma epoch at 0.1 LH scales as observed, contrary to Jeans's (1902) acoustic theory. CMB neutral gas condenses at 300,000 years to Earth-mass ``primordial fog particles'' (PFPs) reflecting the earlier fossil turbulent density and vorticity values. Clumps of PFPs dominate the dark matter of inner galaxy halos, with about 30 million frozen planets per star.
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