English

Hydrodynamics of structure formation in the early Universe

Astrophysics 2009-09-16 v4

Abstract

Theory and observations reveal fatal flaws in the standard LambdaCDM model. The cold dark matter hierarchical clustering paradigm predicts a gradual bottom-up growth of gravitational structures assuming linear, collisionless, ideal flows and unrealistic CDM condensations and mergers. Collisional fluid mechanics with viscosity, turbulence, and diffusion predicts a turbulent big bang and top-down viscous-gravitational fragmentation from supercluster to galaxy scales in the plasma epoch, as observed from 0.3 Gpc void sizes, 1.5 Gpc spins and Kolmogorov-fingerprint-turbulence-signatures in the CMB. Turbulence produced at expanding gravitational void boundaries causes a linear morphology of 3 Kpc fragmenting plasma-protogalaxies along vortex lines, as observed in deep HST images. After decoupling, gas-protogalaxies fragment into primordial-density, million-solar-mass clumps of earth-mass planets forming 0.3 Mpc galactic-dark-matter. White-dwarf-heated planet-atmospheres give dimmed SNe Ia events and false gamma-ray-burst luminosity distances, not dark-energy-Lambda. Quasar microlensing observations rule out no-hair black hole models and require galaxy-dark-matter to be planets-in-clumps.

Keywords

Cite

@article{arxiv.0809.2330,
  title  = {Hydrodynamics of structure formation in the early Universe},
  author = {C. H. Gibson and T. M. Nieuwenhuizen and R. E. Schild},
  journal= {arXiv preprint arXiv:0809.2330},
  year   = {2009}
}

Comments

This paper has been withdrawn because it is superseded by arXiv:0906.5087

R2 v1 2026-06-21T11:19:56.429Z