Einstein-Cartan-Maxwell-Bianchi type-V cosmological models

DOI10.1007/BF00761460zbMath0488.53023OpenAlexW1652744036MaRDI QIDQ1166130

Dieter Lorenz

Publication date: 1982

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

Full work available at URL: https://doi.org/10.1007/bf00761460

zbMATH Keywords

torsionmagnetic fieldEinstein-Cartan theoryspin

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Applications of local differential geometry to the sciences (53B50)

Related Items (1)

A nonsingular, anisotropic universe in a black hole with torsion and particle production

Cites Work

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• Decomposable differential operators in a cosmological context
• Spin and torsion in general relativity. I: Foundations. II: Geometry and field equations
• Topology and cosmology
• Tilted homogeneous cosmological models
• Flat anisotropic models of the universe with torsion and without singularity
• The Large Scale Structure of Space-Time

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