Geodesic completeness of orthogonally transitive cylindrical space–times

DOI10.1063/1.532940zbMath0952.83028arXivgr-qc/9906030OpenAlexW3104748050MaRDI QIDQ4270398

Leonardo Fernández-Jambrina

Publication date: 21 November 1999

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9906030

zbMATH Keywords

spacetimegeodesic completenessperfect fluids

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (4)

Nonsingular G2 stiff fluid cosmologies ⋮ SINGULARITY FREE COSMOLOGICAL SOLUTIONS OF EINSTEIN–MAXWELL EQUATIONS ⋮ STIFF PERFECT FLUID SINGULARITY-FREE DIAGONAL INHOMOGENEOUS COSMOLOGIES IN SCALAR–TENSOR THEORIES ⋮ A SURVEY ON GEODESIC COMPLETENESS OF NONDEGENERATE SUBMANIFOLDS IN SEMI-RIEMANNIAN GEOMETRY

Cites Work

• Spatially homogeneous and inhomogeneous cosmologies with equation of state p=mu
• Singularity theorems and their consequences
• On completeness of certain families of semi-Riemannian manifolds
• Singularity-free cylindrical cosmological model
• Self-graviting fluids with cylindrical symmetry. II
• New class of inhomogeneous cosmological perfect-fluid solutions without big-bang singularity
• Exterior differential system for cosmological perfect fluids and geodesic completeness
• Singularity-free stiff fluid cosmologies
• New non-separable diagonal cosmologies

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