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Related papers: Planets and Dark Energy

200 papers

Migration of dense gaseous clumps that form in young protostellar disks via gravitational fragmentation is investigated to determine the likelihood of giant planet formation. High-resolution numerical hydrodynamics simulations in the…

Solar and Stellar Astrophysics · Physics 2018-10-17 Eduard I. Vorobyov , Vardan Elbakyan

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

The new element of theory of galaxy formation, strong primordial inhomogeneities, is shown to be a reflection of unstable large scale structures of topological defects, created in second order phase transitions in the inflationary Universe.…

Astrophysics · Physics 2007-05-23 M. Yu. Khlopov , S. G. Rubin , A. S. Sakharov

Direct imaging observations constrain the fraction of stars orbited by gas giant planets with separations greater than 10 au to about 0.01 only. This is widely believed to indicate that massive protoplanetary discs rarely fragment on…

Earth and Planetary Astrophysics · Physics 2016-10-07 Sergei Nayakshin

A new mechanism describing the formation of protogalaxies is proposed, which is based on the second- order phase transition in the inflation stage and the domain wall formation upon the end of inflation. The presence of closed domain walls…

High Energy Physics - Phenomenology · Physics 2010-12-09 Sergei G. Rubin , Alexander S. Sakharov , Maxim Yu. Khlopov

Model of supermassive black holes formation inside the clusters of primordial black holes is developed. Namely, it is supposed, that some mass fraction of the universe ~10^-3 is composed of the compact clusters of primordial (relic) black…

Astrophysics · Physics 2009-11-13 V. I. Dokuchaev , Yu. N. Eroshenko , S. G. Rubin

The massive galaxies in the young universe, ten billion years ago, formed stars at surprising intensities. Although this is commonly attributed to violent mergers, the properties of many of these galaxies are incompatible with such events,…

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…

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

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 N. Chandra Wickramasinghe , Jamie H. Wallis , Carl H. Gibson , Rudolph E. Schild

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

[Abridged] Over the past two decades observations and theoretical simulations have established a global frame-work of galaxy formation and evolution in the young Universe. Galaxies formed as baryonic gas cooled at the centres of collapsing…

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

We describe the model of protogalaxy formation around the cluster of primordial black holes with a minimum extension of standard cosmological model. Namely, it is supposed, that a mass fraction of the universe ~10^-3 is composed of the…

Astrophysics · Physics 2007-05-23 Vyacheslav Dokuchaev , Yury Eroshenko , Sergei Rubin

The physical and chemical conditions in young protoplanetary disks set the boundary conditions for planet formation. Although the dust in disks is relatively easily detected as a far-IR photometric ``excess'' over the expected photospheric…

Astrophysics of Galaxies · Physics 2015-05-14 Javier R. Goicoechea , Bruce Swinyard

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.…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Carl H. Gibson , N. Chandra Wickramasinghe , Rudolph E. Schild

The evolution of gravitationally unstable protoplanetary gaseous disks has been studied with the use of three-dimensional smoothed particle hydrodynamics simulations with unprecedented resolution. We have considered disks with initial…

Astrophysics · Physics 2008-11-26 Lucio Mayer , Thomas Quinn , James Wadsley , Joachim Stadel

Recently, it has been observed the extreme metal-poor stars in the Galactic halo, which must be formed just after Pop III objects. On the other hand, the first gas clouds of mass $\sim 10^6 M_{\odot}$ are supposed to be formed at $ z \sim $…

Cosmology and Nongalactic Astrophysics · Physics 2012-04-04 Tetsuya Hara , Shuhei Kunitomo , Masanobu Shigeyasu , Daigo Kajiura

Extreme conditions in natural flows are examined, starting with a turbulent big bang. A hydro-gravitational-dynamics cosmology model is adopted. Planck-Kerr turbulence instability causes Planck-particle turbulent combustion. Inertial-vortex…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-13 R. Norris Keeler , Carl H. Gibson

Eliptical and bulge galaxies share a tight correlation of velocity distribution to both luminosity and black hole mass. There are similar orbital speeds for all galaxies of a given luminosity including dark matter (DM) at large radii. The…

Astrophysics · Physics 2012-07-31 David E. Rosenberg

When black hole jets encounter ambient medium, they can compress the gas, trigger star formation, and create stellar clusters containing tens of thousands of stars. Here, we report a remarkable discovery of such a phenomenon that happened…

Astrophysics of Galaxies · Physics 2025-09-16 Marko Mićić , Themiya Nanayakkara , Xinyu Dai , Jeremy Bailin , Miljan Kolčić