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Related papers: Hydro-Gravitational-Dynamics of Planets and Dark E…

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Self gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the…

Astrophysics · Physics 2008-04-01 Carl H. Gibson , Rudolph E. Schild

From hydro-gravitational cosmology, hydrogen-helium gas planets fragmented at the plasma to gas transition 300,000 years after the big bang in million-star-mass clumps. Stars may form in the clumps by mergers of the planets to make globular…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-30 Carl H. Gibson , Rudolph E. Schild

The standard model for gravitational structure formation in astrophysics, astronomy, and cosmology is questioned. Cold dark matter (CDM) hierarchical clustering cosmology neglects particle collisions, viscosity, turbulence and diffusion and…

Astrophysics · Physics 2007-05-23 Carl H. Gibson

The gravitational hydrodynamics of the primordial plasma with neutrino hot dark matter is considered as a challenge to the bottom-up cold dark matter paradigm. Viscosity and turbulence induce a top-down fragmentation scenario before and at…

Cosmology and Nongalactic Astrophysics · Physics 2009-12-08 Theo M. Nieuwenhuizen , Carl H. Gibson , Rudy E. Schild

From hydro-gravitational-dynamics theory HGD, gravitational structure formation begins 30,000 years after the turbulent big bang by fragmentation into super-cluster-voids and super-clusters. Proto-galaxies in linear and spiral clusters are…

Astrophysics · Physics 2008-09-15 C. H. Gibson , R. E. Schild

The first structures were proto-voids formed in the primordial plasma. Viscous and weak turbulence forces balanced gravitational forces when the scale of causal connection at time 30,000 years matched the viscous and turbulent Schwarz…

Astrophysics · Physics 2007-05-23 Carl H. Gibson

From hydro-gravitational-dynamics theory HGD, gravitational structure formation begins 30,000 years (10^12 s) after the turbulent big bang by viscous-gravitational fragmentation into super-cluster-voids and 10^46 kg…

Cosmology and Nongalactic Astrophysics · Physics 2011-05-10 Carl H. Gibson , Rudy E. Schild

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…

Astrophysics · Physics 2009-09-16 C. H. Gibson , T. M. Nieuwenhuizen , R. E. Schild

Observations are compared to conflicting predictions about self-gravitational structure formation by the hydro-gravitational theory (HGT) of Gibson 1996-2003 versus cold-dark-matter hierarchical-clustering-cosmology (CDMHCC) and the Jeans…

Astrophysics · Physics 2007-05-23 Carl H. Gibson , Rudy Schild

Observations of the interstellar medium by the Herschel, Planck etc. infrared satellites throw doubt on standard {\Lambda}CDMHC cosmological processes to form gravitational structures. According to the Hydro-Gravitational-Dynamics (HGD)…

General Physics · Physics 2012-11-06 Carl H. Gibson

Hydrogravitional-dynamics (HGD) cosmology of Gibson/Schild 1996 predicts proto-globular-star-cluster PGC clumps of Earth-mass planets fragmented from plasma at ~0.3 Myr. Protogalaxies retained the ~0.03 Myr baryonic density existing at the…

Cosmology and Nongalactic Astrophysics · Physics 2011-12-16 Carl H. Gibson , N. Chandra Wickramasinghe , Rudolph E. Schild

The standard model of gravitational structure formation is based on the Jeans 1902 acoustic theory, neglecting crucial effects of viscosity, turbulence and diffusion. A Jeans length scale L_J emerges that exceeds the scale of causal…

Cosmology and Nongalactic Astrophysics · Physics 2011-05-19 Rudolph E. Schild , Carl H. Gibson

Cold dark matter hierarchical clustering (CDMHC) cosmology based on the Jeans 1902 criterion for gravitational instability gives predictions about the early universe contrary to fluid mechanics and observations. Jeans neglected viscosity,…

Astrophysics · Physics 2008-11-26 Carl H. Gibson

The standard model of gravitational structure formation is based on the Jeans 1902 acoustic theory, neglecting nonlinear instabilities controlled by viscosity, turbulence and diffusion. Because the Jeans scale L_J for the hot primordial…

Astrophysics · Physics 2008-09-16 R. E. Schild , C. H. Gibson

Hubble Space telescope (HST) images of merging galaxy system VV29 reveal the 0.3 Mpc baryonic-dark-matter (BDM) halo composed of primordial protoglobularstarcluster (PGC) clumps of planets. Star-cluster-wakes trace the merger by formation…

Astrophysics · Physics 2008-04-01 Carl H. Gibson

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…

Astrophysics · Physics 2007-05-23 Carl H. Gibson

Gravitational hydrodynamics acknowledges that hydrodynamics is essentially nonlinear and viscous. In the plasma, at $z=5100$, the viscous length enters the horizon and causes fragmentation into plasma clumps surrounded by voids. The latter…

Cosmology and Nongalactic Astrophysics · Physics 2010-03-03 Theo M. Nieuwenhuizen , Carl H. Gibson , Rudolph E. Schild

Matter in the universe has become ``dark'' or ``missing'' through misconceptions about the fluid mechanics of gravitational structure formation. Gravitational condensation occurs on non-acoustic density nuclei at the largest Schwarz length…

Astrophysics · Physics 2007-05-23 Carl H. Gibson

Gravitational instability (GI) has long been considered a viable pathway for giant planet formation in protoplanetary disks (PPDs), especially at wide orbital separations or around low-mass stars where core accretion faces significant…

Earth and Planetary Astrophysics · Physics 2025-10-24 Yang Ni , Hongping Deng , Xue-Ning Bai

We study thermal-gravitational instability in simplified models for protogalactic halos using three-dimensional hydrodynamic simulations. The simulations followed the evolution of gas with radiative cooling down to T = 10^4 K, background…

Astrophysics · Physics 2009-11-11 Chang Hyun Baek , Hyesung Kang , Jongsoo Kim , Dongsu Ryu
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