Spherically symmetric T-models in the general theory of relativity

DOI10.1023/A:1002779702615zbMath0979.83015MaRDI QIDQ5943144

V. A. Ruban

Publication date: 19 February 2002

Published in: General Relativity and Gravitation (Search for Journal in Brave)

zbMATH Keywords

dustlike matterFriedmann modelmass defect

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Equations of motion in general relativity and gravitational theory (83C10) History of relativity and gravitational theory (83-03)

Related Items (1)

\(N\)-spheres in general relativity: regular black holes without apparent horizons, static wormholes with event horizons and gravastars with a tube-like core

Cites Work

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• Relativistic Cosmology
• Effect of Inhomogeneity on Cosmological Models
• Spherically Symmetric Gravitational Fields
• SPHERICALLY SYMMETRIC DISTRIBUTIONS OF MATTER WITHOUT PRESSURE
• Problems of relativistic cosmology
• On Continued Gravitational Contraction
• Spherically Symmetrical Models in General Relativity
• Cosmological Application of Relativity

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