Add to ORKGInternational audienceThe most widely accepted model of Solar System formation, known as the Nebular hypothesis, does not solve the Angular Momentum problem—why is the orbital momentum of Jupiter larger than rotational momentum of the Sun? The present manuscript introduces a Rotational Fission model of creation and evolution of Macrostructures of the World (Superclusters, Galaxies, Extrasolar Systems), based on Overspinning Cores of the World’s Macroobjects, and the Law of Conservation of Angular Momentum. The Hypersphere World-Universe model is the only cosmological model in existence that is consistent with this Fundamental Law
We study the stellar angular momentum of thousands of galaxies in the Illustris cosmological simulat...
Context. Giant planets orbiting main-sequence stars closer than 0.1 AU are called hot Jupiters. They...
Abstract: The law of conservation of angular momentum, which controls Planck’s constant, plays a fun...
Theoretical models of the formation of the solar system are examined critically in a review focusing...
Angular momentum in our solar system is largely distributed between the Sun’s rotation and the plane...
The rotational angular momentum of an asteroid or planet and the average orbital angular momentum of...
We discuss the equation of motion of the rotating homogenous and isotropic model of the Universe. We...
The determination of the specific angular momentum radial profile, j(r), in the early stages of star...
International audienceContext. Rotation plays a key role in the star-formation process, from pre-ste...
Context. Galaxy formation in the current cosmological paradigm is a very complex process in which in...
© 2016 World Scientific Publishing Company We consider collision of two particles in rotating spacet...
A new approach has been used to evaluate the momentum and angular momentum of the isotropic and homo...
Planar orbital theory is developed from the concept of the conserved angular momentum of spacetime i...
The formation of compact objects such as stars and black holes is strongly constrained by the requir...
Thesis (M.S.)--Massachusetts Institute of Technology, Dept. of Meteorology, 1964.Includes bibliograp...
We study the stellar angular momentum of thousands of galaxies in the Illustris cosmological simulat...
Context. Giant planets orbiting main-sequence stars closer than 0.1 AU are called hot Jupiters. They...
Abstract: The law of conservation of angular momentum, which controls Planck’s constant, plays a fun...
Theoretical models of the formation of the solar system are examined critically in a review focusing...
Angular momentum in our solar system is largely distributed between the Sun’s rotation and the plane...
The rotational angular momentum of an asteroid or planet and the average orbital angular momentum of...
We discuss the equation of motion of the rotating homogenous and isotropic model of the Universe. We...
The determination of the specific angular momentum radial profile, j(r), in the early stages of star...
International audienceContext. Rotation plays a key role in the star-formation process, from pre-ste...
Context. Galaxy formation in the current cosmological paradigm is a very complex process in which in...
© 2016 World Scientific Publishing Company We consider collision of two particles in rotating spacet...
A new approach has been used to evaluate the momentum and angular momentum of the isotropic and homo...
Planar orbital theory is developed from the concept of the conserved angular momentum of spacetime i...
The formation of compact objects such as stars and black holes is strongly constrained by the requir...
Thesis (M.S.)--Massachusetts Institute of Technology, Dept. of Meteorology, 1964.Includes bibliograp...
We study the stellar angular momentum of thousands of galaxies in the Illustris cosmological simulat...
Context. Giant planets orbiting main-sequence stars closer than 0.1 AU are called hot Jupiters. They...
Abstract: The law of conservation of angular momentum, which controls Planck’s constant, plays a fun...