Non-radiative solutions of Einstein's equations for dust

DOI10.1007/BF01617918zbMath0337.53030MaRDI QIDQ1230424

W. B. Bonnor

Publication date: 1976

Published in: Communications in Mathematical Physics (Search for Journal in Brave)

Mathematics Subject Classification ID

Local differential geometry (53B99)

Related Items (18)

Covariant energy-momentum and an uncertainty principle for general relativity ⋮ GENERALIZED STRONG CURVATURE SINGULARITIES AND COSMIC CENSORSHIP ⋮ Review on exact and perturbative deformations of the Einstein-Straus model: uniqueness and rigidity results ⋮ Frame rotation in the Szekeres spacetimes ⋮ Axially symmetric static sources of gravitational field ⋮ Newtonian analogs of Szekeres' space-times ⋮ Spacetime junctions and the collapse to black holes in higher dimensions ⋮ SPACE–TIME ENERGY–MOMENTUM, THE OBSERVER AND UNCERTAINTY IN GENERAL RELATIVITY ⋮ Thermodynamic class II Szekeres–Szafron solutions. Singular models ⋮ Energy distributions of the Szekeres universes in teleparallel gravity ⋮ On the global visibility of the singularity in quasi-spherical collapse. ⋮ Influence of intrinsic spin in the formation of singularities for inhomogeneous effective dust space-times ⋮ Intrinsic conformal symmetries in Szekeres models ⋮ Spacetimes with continuous linear isotropies. I: Spatial rotations ⋮ About vacuum solutions of Einstein’s field equations with flat three-dimensional hypersurfaces ⋮ The Szekeres swiss cheese model and the CMB observations ⋮ The role of energy and a new approach to gravitational waves in general relativity ⋮ The Curzon singularity. II: Global picture

Cites Work

• A class of inhomogeneous cosmological models
• Effect of Inhomogeneity on Cosmological Models

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