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Gravitation and Cosmology

, Volume 18, Issue 2, pp 107–112 | Cite as

Induced antigravity in extended general relativity

  • Y. A. RylovEmail author
Article

Abstract

An extension of general relativity to non-Riemannian geometries suitable for description of the space-time geometry leads to integral dynamic equations which are valid for continuous and discrete space-times. The gravitational field of a homogeneous heavy non-rotating sphere is calculated inside the sphere. The space-time geometry appears to be non-Riemannian. In the case where the gravitational radius of the sphere is of the order of its own radius, an induced antigravity appears inside the sphere. In other words, the gravitational force inside the sphere appears to be directed from the center. The antigravity resists to a collapse of the sphere and to black hole formation.

Keywords

Black Hole Gravitational Force Dust Cloud World Line Additional Particle 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Pleiades Publishing, Ltd. 2012

Authors and Affiliations

  1. 1.Institute for Problems in MechanicsRussian Academy of SciencesMoscowRussia

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