Turbulent mixing, viscosity, diffusion, and gravity in the formation of cosmological structures: The fluid mechanics of dark matter

被引:16
|
作者
Gibson, CH [1 ]
机构
[1] Univ Calif San Diego, Ctr Astrophys & Space Sci, Dept MAE, La Jolla, CA 92093 USA
[2] Univ Calif San Diego, Ctr Astrophys & Space Sci, Dept SIO, La Jolla, CA 92093 USA
关键词
turbulence; mixing; fluid mechanics; gravitational instability; cosmology; astrophysics;
D O I
10.1115/1.1319156
中图分类号
TH [机械、仪表工业];
学科分类号
0802 ;
摘要
Self-gravitational structure formation theory for astrophysics and cosmology is revised using nonlinear fluid mechanics. Gibson's 1996-2000 theory balances fluid mechanical forces with gravitational forces and density diffusion with gravitational diffusion at critical viscous, turbulent, magnetic, and diffusion length scales termed Schwarz scales. Condensation and fragmentation occur for scales exceeding the largest Schwarz scale rather than L-J, the length scale introduced by Jeans in his 1902 inviscid-linear-acoustic theory. The largest Schwarz scale is often larger or smaller than L-J. From the new theory, the inner-halo (10(21) m) dark-matter of galaxies comprises similar to 10(5) fossil-L-J-scale clumps of 10(12) Earth-mass fossil-L-SV-scale planets railed primordial fog particles (PFPs) condensed soon after the cooling transition from plasma to neutral gas, 300,000 years after the Big Bang, with PFPs tidally disrupted from their clumps forming the interstellar medium. PFPs explain Schild's 1996 "rogue planers.., likely to be the missing mass" of a quasar lens-galaxy, inferred from twinkling frequencies of the quasar mirages, giving 30 million planets per star. The non-baryonic dark matter is super-diffusive and fragments at large L-SD scales to form massive outer-galaxy-halos. In the beginning of structure formation 30,000 years after the Big Bang, with photon viscosity values nu of 5 x 10(26) m(2) s(-1) the viscous Schwarz scale matched the horizon scale (L(SV)approximate toL(H)<L-J), giving 10(46) kg proto-superclusters and finally 10(42) kg proto-galaxies. Non-baryonic fluid diffusivities D<similar to> 10(28) m(2) s(-1) from galaxy-outer-halo (L-SD) scales (10(22) m) measured in a dense galaxy cluster by Tyson, J. A., and Fischer, P., 1995, "Measurement of the Mass profile of Abell 1689," Ap. J., 446, pp. L55-L58, indicate non-baryonic dark matter particles must have small mass (similar to 10(-35) kg) to avoid detection.
引用
收藏
页码:830 / 835
页数:6
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