Dust universes with spatial spherical symmetry and Euclidean initial hypersurfaces

DOI10.1007/BF02352677zbMath0615.76132MaRDI QIDQ1820989

Ettore Laserra

Publication date: 1985

Published in: Meccanica (Search for Journal in Brave)

zbMATH Keywords

general relativityspherically symmetric dustEuclidean initial hypersurfacepressure-free spherically symmetric systems of particlesTolman-Bondi equations

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (8)

THE WEIERSTRASS CRITERION AND THE LEMAÎTRE–TOLMAN–BONDI MODELS WITH COSMOLOGICAL CONSTANT Λ ⋮ Evolution of dust shells in Tolman-Bondi space-time according to the Weierstrass approach ⋮ On the evolution of dust shells in Lemaître-Tolman-Bondi models ⋮ On geometrical and physical consequences of using certain special classes of comoving physical frames of reference ⋮ Fractal Cantorian structures with spatial pseudo-spherical symmetry for a possible description of the actual segregated universe as a consequence of its primordial fluctuations ⋮ On the mechanical analogy between the relativistic evolution of a spherical dust universe and the classical motion of falling bodies ⋮ A REVIEW ON THE GEOMETRIC FORMULATION OF TOLMAN–BONDI EQUATIONS IN GENERAL RELATIVITY ⋮ Analysis of Lemaître-Tolman-Bondi Cosmological Models in a Short Range Collapse/Generation Interval by a Puiseux Series

Cites Work

• Proiezioni naturali e derivazione trasversa in una varietà riemanniana a metrica iperbolica normale
• L'intégration des équations de la gravitation relativiste et le problème des \(n\) corps
• Effect of Inhomogeneity on Cosmological Models
• Spherically Symmetrical Models in General Relativity
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