Physics – Fluid Dynamics
Scientific paper
Nov 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..dfd.ar001c&link_type=abstract
American Physical Society, 58th Annual Meeting of the Division of Fluid Dynamics, November 20-22, 2005, abstract #AR.001
Physics
Fluid Dynamics
Scientific paper
The first turbulence was the strongly exothermic turbulent combustion that produced the big bang (1). Strong force freeze-out by quark-gluon-viscous forces damped the turbulence and inflated space (2). The second turbulence occurred in the plasma epoch, triggered by the expansion of space and gravitational fragmentation of the H-He plasma into proto-supercluster-voids. Proto-galaxies formed in chains just before the transition to gas, reflecting viscous straining along vortex lines, where maximum positive rate-of-strain plus the positive straining of the expanding universe stretched and separated proto-galaxies caused by gravity and maximum negative rate-of-strain compression opposing universe expansion. The dim most distant galaxies revealed by the Hubble Space Telescope (figure) are in chains of clumps (3) with ˜1500 times more dark matter (planets) than luminous matter (stars). See figure at http://www-acs.ucsd.edu/˜ir118 1. Gibson, C. H., ``The First Turbulent Combustion,'' Combustion Science and Technology, 177: 1049--1071, 2005 2. Gibson, C. H., ``The first turbulence and the first fossil turbulence.'' Flow Turbulence and Combustion, 72, 161--179, 2004 3. Elmegreen, D. M. et al., ``Chain galaxies '', ApJ 603:75, 2004
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