Interacting Cosmic Fluids in Brans-Dicke Cosmology
arXiv:1005.0062 · doi:10.1142/S0217732310033499
Abstract
We provide a detailed description for power-law scaling FRW cosmological models in Brans-Dicke theory dominated by two interacting fluid components during the expansion of the universe.
arXiv comment13 pages, 8 figures
References in corpus (7)
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Supernova Limits on the Cosmic Equation of State
- Time Dependence of Brans-Dicke Parameter w for an Expanding Universe
- Cosmic Evolution in Generalised Brans-Dicke Theory
- Interacting cosmic fluids in power-law Friedmann-Robertson-Walker cosmological models
- Generalized Brans-Dicke cosmology in the presence of matter and dark energy
- Inflationary cosmology with two-component fluid and thermodynamics
Cited by in corpus (15)
- Stability Analysis in Tachyonic Potential Chameleon cosmology
- Attractors, Statefinders and Observational Measurement for Chameleonic Brans--Dicke Cosmology
- Two-fluid evolving Lorentzian wormholes
- Stability analysis and Observational Measurement in Chameleonic Generalised Brans--Dicke Cosmology
- Phantom evolving wormholes with big rip singularities
- A new approach in stability analysis: case study: tachyon cosmology with non-minimally coupled scalar field-matter
- Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
- Canonical and phantom scalar fields as an interaction of two perfect fluids
- Entropy and statefinder diagnosis in chameleon cosmology
- Stability analysis in Modified Non-Local Gravity
- Stability analysis and observational constraints in scalar tensor theory
- Observational constraints in scalar tensor theory with tachyonic potential
- Radiation in (2+1)-dimensions
- Constraints on scalar-tensor theories from observations
- Geometric and thermodynamic properties in Gauss-Bonnet gravity