Physics – Fluid Dynamics
Scientific paper
Nov 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aps..dfd..fb01g&link_type=abstract
American Physical Society, Division of Fluid Dynamics Meeting, November 21-23, 1999 New Orleans, LA, abstract #FB.01
Physics
Fluid Dynamics
Scientific paper
Jeans's (1902) acoustic theory of gravitational condensation is commonly used, but is unreliable. Gibson's (1996-1999) theory balances fluid and gravitational forces and diffusion and gravitational velocities at turbulent, viscous, and diffusive L_ST,SV,SD Schwarz instability scales that were much smaller than LJ in the quiet, super-viscous, expanding universe soon after the Big Bang. Thus, both turbulence and structure formation began with proto- supercluster-voids in the hot plasma epoch at about 30,000 years when the Kolmogorov scale LK and L_SV both decreased to match the increasing Hubble (horizon) scale LH = ct, where c is light speed and t is time. Viscous-turbulent fragmentation decreased with cooling to proto-galaxy masses just before the plasma formed neutral H-He gas at 300,000 years. Observations of δ T/T <= 10-5 at 0.1 LH in the cosmic microwave background also imply this early viscous and buoyancy damping of the primordial turbulence. All the neutral gas then condensed to form Earth-mass hydrogenous planetoids that persist as the dominant galactic dark matter, observed near hot stars by the HST and by Schild (1996) in a twin- image-quasar galaxy lens as ``rogue planets ... likely to be the missing mass''. Observed super-cluster-halo scales suggest non-baryonic dark matter from the large implied L_SD values. See astro-ph and the author's webpage.
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