Turbulent Gravitational Instability and Dark Matter

Physics – Fluid Dynamics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Sir James Jeans (1902, 1929) theory of gravitational condensation gives vast errors, as expected from linear theories applied to nonlinear processes. A new theory using Kolmogorov turbulence methods shows non-acoustic density extrema and saddle points produced by turbulence are gravitationally unstable at turbulent, viscous, or diffusive Schwarz scales L_ST,V,D independent of L_J. At these scales density moves up density gradients as though its diffusivity were negative, so maxima concentrate and minima become voids. Thus, structure formation began with 10^46 kg proto-superclusters in the hot plasma epoch 13,000 years after the Big Bang when L_SV decreased to the Hubble (horizon) scale LH = ct, where c is light speed and t is time, and decreased further to 10^42 kg proto-galaxies just before the cooled plasma formed neutral H-He gas at 300,000 years. In 10^3 years the gas condensed to 10^23 - 10^25 kg L_SV - L_ST scale objects termed ``primordial fog particles'' (PFPs) that persist as the galactic ``dark matter'' objects observed by Schild (1996) in a twin-image-quasar galaxy lens as ``rogue planets ... likely to be the missing mass''. See Gibson/Schild preprint on webpage.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Turbulent Gravitational Instability and Dark Matter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Turbulent Gravitational Instability and Dark Matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Turbulent Gravitational Instability and Dark Matter will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1686103

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.