Anisotropic universe models with perfect fluid and dark energy with time varying G and \(\Lambda \)
From MaRDI portal
Publication:445271
DOI10.1007/s10773-012-1146-2zbMath1248.83108OpenAlexW2023802350MaRDI QIDQ445271
V. Fayaz, F. Felegary, Hossien Hossienkhani
Publication date: 24 August 2012
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-012-1146-2
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)
Related Items
Binary mixture of perfect fluid and dark energy in modified theory of gravity ⋮ Instability of interacting ghost dark energy model in an anisotropic universe
Cites Work
- Generalized chaplygin gas model: Cosmological consequences and statefinder diagnosis
- Interacting new agegraphic viscous dark energy with varying \(G\)
- Bulk-brane interaction and holographic dark energy
- Holographic Chaplygin gas model
- A generalisation of the Heckmann-Schücking cosmological solution
- A model to explain varying \(\Lambda\), \(G\) and \(\sigma^{2}\) simultaneously
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- HOLOGRAPHIC CHAPLYGIN DGP COSMOLOGIES
- Role of modified Chaplygin gas in accelerated universe
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- An alternative to quintessence
