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相关论文: Cold dark matter cosmology conflicts with fluid me…

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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…

天体物理学 · 物理学 2007-05-23 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…

天体物理学 · 物理学 2008-09-16 R. E. Schild , C. H. Gibson

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…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson , Rudy Schild

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…

天体物理学 · 物理学 2008-08-26 Carl H. Gibson , Rudolph E. 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)…

综合物理 · 物理学 2012-11-06 Carl H. Gibson

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…

宇宙学与河外天体物理 · 物理学 2011-05-19 Rudolph E. Schild , Carl H. Gibson

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…

天体物理学 · 物理学 2009-09-16 C. H. Gibson , T. M. Nieuwenhuizen , R. E. Schild

Jeans's (1902 & 1929) linear gravitational instability criterion gives truly spectacular errors in its predictions of cosmological structure formation according to Gibson's (1996) new nonlinear theory. Scales are determined by viscous or…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

In the standard cosmological model a mysterious cold dark matter (CDM) component dominates the formation of structures. Numerical studies of the formation of CDM halos have produced several robust results that allow unique tests of the…

宇宙学与河外天体物理 · 物理学 2015-05-13 Jürg Diemand , Ben Moore

Cold Dark Matter (CDM) has become the standard modern theory of cosmological structure formation. Its predictions appear to be in good agreement with data on large scales, and it naturally accounts for many properties of galaxies. But…

天体物理学 · 物理学 2009-11-07 Joel R. Primack

Observations of quasar microlensing by Schild 1996 show the baryonic dark matter BDM of galaxies is micro-brown-dwarfs, primordial hydrogen-helium planets formed at the plasma to gas transition 10^13 seconds, in trillion-planet clumps…

地球与行星天体物理 · 物理学 2011-03-08 Carl H. Gibson

The concordance cosmological model based on cold dark matter makes definitive predictions for the growth of galaxies in the Universe, which are being actively studied using numerical simulations. These predictions appear to contradict the…

天体物理学 · 物理学 2015-06-24 Oleg Y. Gnedin

The cold dark matter (CDM) cosmological model has been remarkably successful in explaining cosmic structure over an enormous span of redshift, but it has faced persistent challenges from observations that probe the innermost regions of dark…

宇宙学与河外天体物理 · 物理学 2016-09-07 David H. Weinberg , James S. Bullock , Fabio Governato , Rachel Kuzio de Naray , Annika H. G. Peter

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…

宇宙学与河外天体物理 · 物理学 2011-12-16 Carl H. Gibson , N. Chandra Wickramasinghe , Rudolph E. Schild

The conventional cold, particle interpretation of dark matter (CDM) still lacks laboratory support and struggles with the basic properties of common dwarf galaxies, which have surprisingly uniform central masses and shallow density…

星系天体物理 · 物理学 2014-06-26 Hsi-Yu Schive , Tzihong Chiueh , Tom Broadhurst

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…

天体物理学 · 物理学 2008-04-01 Carl H. Gibson , Rudolph E. Schild

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…

宇宙学与河外天体物理 · 物理学 2010-03-03 Theo M. Nieuwenhuizen , Carl H. Gibson , Rudolph E. Schild

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…

宇宙学与河外天体物理 · 物理学 2009-12-08 Theo M. Nieuwenhuizen , Carl H. Gibson , Rudy E. Schild

Cold Dark Matter (CDM) has become the standard modern theory of cosmological structure formation. Its predictions appear to be in good agreement with data on large scales, and it naturally accounts for many properties of galaxies. But…

天体物理学 · 物理学 2007-05-23 Joel R. Primack

The cold dark matter (CDM) cosmological model unambigously predicts that a large number of haloes should survive as subhaloes when they are accreted into a larger halo. The CDM model would be ruled out if such substructures were shown not…

宇宙学与河外天体物理 · 物理学 2016-04-27 Ran Li , Carlos S. Frenk , Shaun Cole , Liang Gao , Sownak Bose , Wojciech A. Hellwing
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