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Hydrogravitional-dynamics (HGD) cosmology of Gibson/Schild 1996 predicts that the primordial H-He^4 gas of big bang nucleosynthesis became proto-globular-star-cluster clumps of Earth-mass planets at 300 Kyr. The first stars formed from…

宇宙学与河外天体物理 · 物理学 2015-05-30 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…

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 origin of life and the origin of the universe are among the most important problems of science and they might be inextricably linked. Hydro-gravitational-dynamics (HGD) cosmology predicts hydrogen-helium gas planets in clumps as the…

宇宙学与河外天体物理 · 物理学 2015-05-18 Carl H. Gibson , Rudolph E. Schild , N. C. Wickramasinghe

A key result of hydrogravitational dynamics cosmology relevant to astrobiology is the early formation of vast numbers of hot primordial-gas planets in million-solar-mass clumps as the dark matter of galaxies and the hosts of first life.…

宇宙学与河外天体物理 · 物理学 2015-05-19 Carl H. Gibson , N. Chandra Wickramasinghe , Rudolph E. Schild

We explore the conditions prevailing in primordial planets in the framework of the HGD cosmologies as discussed by Gibson and Schild. The initial stages of condensation of planet-mass H-4He gas clouds in trillion-planet clumps is set at…

宇宙学与河外天体物理 · 物理学 2015-05-19 N. Chandra Wickramasinghe , Jamie H. Wallis , 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

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…

宇宙学与河外天体物理 · 物理学 2010-12-30 Carl H. Gibson , Rudolph E. Schild

At early times the Universe was filled up with an extremely dense and hot gas. Due to the expansion it cooled below the binding energies of atoms which led to the formation of the first nuclei. In the physical environment of the…

天体物理学 · 物理学 2007-05-23 Denis Puy

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

We describe results from a fully self-consistent three dimensional hydrodynamical simulation of the formation of one of the first stars in the Universe. Dark matter dominated pre-galactic objects form because of gravitational instability…

天体物理学 · 物理学 2011-06-15 Tom Abel , Greg L. Bryan , Michael L. Norman

Recent spacecraft observations exploring solar system properties impact standard paradigms of the formation of stars, planets and comets. We stress the unexpected cloud of microscopic dust resulting from the DEEP IMPACT mission, and the…

宇宙学与河外天体物理 · 物理学 2010-12-30 Rudolph E. Schild , Carl H. Gibson

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

The transformation of organic molecules into the simplest self-replicating living system,a microorganism, is accomplished from a unique event or rare events that occurred early in the Universe. The subsequent dispersal on cosmic scales and…

宇宙学与河外天体物理 · 物理学 2010-03-02 Carl H. Gibson , N. Chandra Wickramasinghe

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

The first bound star-forming systems in the universe are predicted to form at redshifts of about 30 and to have masses of the order of 10^6 M_sun. Although their sizes and masses are similar to those of present star-forming regions, their…

天体物理学 · 物理学 2007-05-23 Richard B. Larson

The first stars in the Universe are predicted to have been much more massive than the Sun. Gravitational condensation accompanied by cooling of the primordial gas due to molecular hydrogen, yields a minimum fragmentation scale of a few…

天体物理学 · 物理学 2009-07-09 Volker Bromm , Abraham Loeb

The formation of the first generations of stars at redshifts z > 15-20 signaled the transition from the simple initial state of the universe to one of increasing complexity. We here review recent progress in understanding the assembly…

天体物理学 · 物理学 2009-11-13 Jarrett L. Johnson , Thomas H. Greif , Volker Bromm

We describe high resolution Smoothed Particle Hydrodynamics (SPH) simulations of three approximately $M_*$ field galaxies starting from \LCDM initial conditions. The simulations are made intentionally simple, and include photoionization,…

天体物理学 · 物理学 2009-11-11 Thorsten Naab , Peter H. Johansson , Jeremiah P. Ostriker , George Efstathiou

In the redshift range 100<(1+z)<137, the cosmic microwave background (CMB) had a temperature of 273-373K (0-100 degrees Celsius), allowing early rocky planets (if any existed) to have liquid water chemistry on their surface and be…

宇宙学与河外天体物理 · 物理学 2015-06-18 Abraham Loeb

Cosmic structure originated from minute density perturbations in an almost homogeneous universe. The first stars are believed to be very massive and luminous, providing the first ionizing radiation and heavy elements to the universe and…

天体物理学 · 物理学 2008-04-28 John H. Wise
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