Non-existence of Bianchi type-1 perfect fluid cosmological models in a bi-metric theory of gravitation

DOI10.1007/BF00637454zbMath0675.76122MaRDI QIDQ1122451

S. H. Smith

Publication date: 1989

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

perfect fluid distributionanisotropic Bianchi type-I cosmological modelsvacuum cosmological model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (12)

Inhomogeneous plane symmetric string cosmological models in bimetric theory ⋮ Bianchi types V and \(\text{VI}_{0}\) cosmic strings coupled with Maxwell fields in bimetric theory ⋮ On Kantowski-Sachs cosmological models in bimetric theory of gravity ⋮ On plane symmetric domain walls and cosmic strings in bimetric theory ⋮ \(N\)-dimensional string cosmological model in Brans-Dicke theory of gravitation ⋮ On axially symmetric domain walls and cosmic strings in bimetric theory ⋮ On Kantowski-Sachs cosmic strings coupled with Maxwell fields in bimetric relativity ⋮ Charged fluid sphere in bimetric general theory of relativity ⋮ Bianchi type-III cosmological model in four- and five-dimensional bimetric theory of relativity ⋮ Higher Dimensional Cosmological Model in Brans-Dicke Theory of Gravitation-I ⋮ Spherically symmetric cosmic strings in bimetric theory ⋮ Non-existence of \(N\)-dimensional static plane symmetric solutions in bimetric relativity theory

Cites Work

• A bi-metric theory of gravitation

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