NON-NEWTONIAN BEHAVIOR IN WEAK FIELD GENERAL RELATIVITY FOR EXTENDED ROTATING SOURCES

DOI10.1142/S0218271808012140zbMath1164.83002arXivastro-ph/0602519OpenAlexW2167358718MaRDI QIDQ3532161

Herbert Balasin, Daniel Grumiller

Publication date: 3 November 2008

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0602519

zbMATH Keywords

dark mattergalactic rotation curvesaxially-symmetric stationary perfect fluid solutions in general relativity

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (7)

Galactic dynamics in general relativity: the role of gravitomagnetism ⋮ Rigid rotation in GR and a generalization of the virial theorem for gravitomagnetism ⋮ Gravitomagnetism and galaxy rotation curves: a cautionary tale ⋮ Low energy limits of general relativity and galactic dynamics ⋮ Testing Basic Laws of Gravitation – Are Our Postulates on Dynamics and Gravitation Supported by Experimental Evidence? ⋮ The effect of spacetime curvature on statistical distributions ⋮ Conformally-flat, non-singular static metric in infinite derivative gravity

Cites Work

• The universe seen at different scales
• Information Entropy in Cosmology
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Astrophysical constraints on modifying gravity at large distances
• Cosmological Solutions in Macroscopic Gravity
• IX.—The Gravitational Field of a Distribution of Particles Rotating about an Axis of Symmetry
• General Relativity

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