Newtonian-like and anti-Newtonian universes

DOI10.1088/0264-9381/15/4/021zbMath0940.83015arXivgr-qc/9802014OpenAlexW3104488133WikidataQ63390708 ScholiaQ63390708MaRDI QIDQ4699647

Roy Maartens, W. M. Lesame, George F. R. Ellis

Publication date: 18 November 1999

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9802014

zbMATH Keywords

Weyl tensorgeneral relativityintegrability conditionslinearized Einstein equationslinearization instabilityirrotational dust spacetimesvanishing electric partvanishing magnetic part

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (14)

Gravitational radiation, vorticity and the electric and magnetic part of Weyl tensor ⋮ Cylindrically symmetric relativistic fluids and the purely electric Weyl tensor ⋮ Irrotational-fluid cosmologies in fourth-order gravity ⋮ A prediction for anisotropies in the nearby Hubble flow ⋮ Modelling the emergence of cosmic anisotropy from non-linear structures ⋮ Bianchi type-V cosmological model with purely magnetic solution ⋮ Energetics of the Einstein-Rosen spacetime ⋮ Nonlinear gravito-electromagnetism ⋮ An example of non-Weyl preserving complex transformation ⋮ Investigations of \(f(R)\)-gravity counterparts of the general relativistic shear-free conjecture by illustrative examples ⋮ Perfect fluid spacetimes with a purely magnetic Weyl tensor ⋮ Integrability conditions of quasi-Newtonian cosmologies in modified gravity ⋮ Bianchi type VI₀ cosmology with purely magnetic and purely electric space time ⋮ Shear-free perfect fluids in general relativity: Gravito-magnetic spacetimes

This page was built for publication: Newtonian-like and anti-Newtonian universes