Two-fluid anisotropic cosmological model with variable \(G\) and \(\varLambda\)
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Publication:395533
DOI10.1007/S10773-013-1715-ZzbMath1282.83081OpenAlexW2047375267MaRDI QIDQ395533
Publication date: 29 January 2014
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-013-1715-z
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Cites Work
- Bulk viscous Bianchi-III models with time dependent \(G\) and \(\Lambda \)
- Bulk viscous fluid hypersurface-homogeneous cosmological models with time varying G and \(\Lambda \)
- Two-fluid cosmological models in Bianchi type-V space-time
- Cosmology of general relativity without energy-momentum conservation
- Universe with time dependent deceleration parameter and \(\Lambda\) term in general relativity
- A critical density cosmological model with varying gravitational and cosmological ``constants
- Static universe in a modified Brans-Dicke cosmology
- Two-fluid cosmological models in a Bianchi type I space-times
- Thermodynamics and two-fluid cosmological models
- Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
- Two-fluid Bianchi type II cosmological models
- Bianchi type I cosmological models with variable \(G\) and \(\Lambda\): A comment
- Two-fluid cosmological model of Bianchi type-V with negative constant deceleration parameter
- A study of angular size-redshift relation for models in which Λ decays as the energy density
- Consequences on variable Λ-models from distant type Ia supernovae and compact radio sources
- The Cosmological Implications of the Recent Counts of Radio Sources: II. An Evolutionary Model
- Early viscous universe with variable gravitational and cosmological ‘constants’
- Two-fluid cosmological models
- Order-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>R</mml:mi></mml:math>Vacuum Action Functional in Scalar-Free Unified Theories with Spontaneous Scale Breaking
- A Machian model of dark energy
- Cosmic acceleration with a positive cosmological constant
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- The Cosmological Constants
- A new basis for cosmology
- Cosmology with self-adjusting vacuum energy density from a renormalization group fixed point
- Study of the magnitude-redshift relation for type Ia supernovae in a model resulting from a Ricci-symmetry
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