Perfect fluid Bianchi I model with variable \(G\) and \(\Lambda \)
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Publication:844847
DOI10.1134/S0202289309040045zbMath1181.83155OpenAlexW1970870680WikidataQ125889255 ScholiaQ125889255MaRDI QIDQ844847
Publication date: 5 February 2010
Published in: Gravitation \& Cosmology (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0202289309040045
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
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- About Bianchi I with VSL
- Bulk viscous cosmological models with variable \(G\) and \(\Lambda\)
- Bianchi type I viscous universe with variable \(G\) and \(\Lambda\)
- Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
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- Ricci and matter collineations in space-time
- Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant
- A model to explain varying \(\Lambda\), \(G\) and \(\sigma^{2}\) simultaneously
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- A class of homogeneous cosmological models
- Symmetries of Bianchi I space–times
- The cosmological constant and dark energy
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- Self-similar spatially homogeneous cosmologies: orthogonal perfect fluid and vacuum solutions
- Algebraic invariants of the Riemann tensor in a four-dimensional Lorentzian space
- Matter collineations: The inverse ‘‘symmetry inheritance’’ problem
- Kinematic self-similarity
- On the Relation between the Expansion and the Mean Density of the Universe
- Exact Solutions of Einstein's Field Equations
- Spherically symmetric spacetimes and kinematic self-similarity
- Kinematic self-similar locally rotationally symmetric models
- Self-similarity in general relativity
- The Weyl tensor in spatially homogeneous cosmological models
- BIANCHI I WITH VARIABLE G AND Λ: SELF-SIMILAR APPROACH
- Self-Similar Solutions as Intermediate Asymptotics
- SYMMETRIES OF LOCALLY ROTATIONALLY SYMMETRIC MODELS
- A new basis for cosmology
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