Cosmic shear in inflationary models of Bianchi types VIII and IX

DOI10.1007/BF00640002zbMath0629.76137MaRDI QIDQ1094295

Harald H. Soleng

Publication date: 1987

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

zbMATH Keywords

inflationary eraexact solutionsinitial conditionsBianchi type-VIII modelsgroup structuresvacuum fluidanisotropic expansionEinstein's field equations of vacuumscalar field with an almost constant potential

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 (7)

Junction conditions and static fluid cylinders in Lyra's geometry ⋮ Higher dimensional FRW cosmological models in self-creation theory ⋮ The Vaidya–Patel solution with Robertson–Walker metric as a rotating inflationary scenario ⋮ Exact Bianchi-type VIII and IX models in the presence of the self- creation theory of cosmology ⋮ Axially symmetric Bianchi type-I model with massless scalar field and cosmic strings in Barber's self-creation cosmology ⋮ Plane symmetric string cosmological model in modified theory of general relativity ⋮ Magnetized anisotropic dark energy models in Barber's second self-creation theory

Cites Work

• Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant
• Inflationary universe: A possible solution to the horizon and flatness problems
• An Example of a New Type of Cosmological Solutions of Einstein's Field Equations of Gravitation

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