INTERACTING COSMIC FLUIDS IN BRANS–DICKE COSMOLOGY

DOI10.1142/S0217732310033499zbMath1202.83132arXiv1005.0062MaRDI QIDQ3062805

Hamed Amiri, Narges Mohamadi, Hossein Farajollahi

Publication date: 28 December 2010

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1005.0062

zbMATH Keywords

expansioninflationscalar fieldinteractionBrans-Dicke cosmologyphantomdark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)

Related Items (6)

Canonical and phantom scalar fields as an interaction of two perfect fluids ⋮ Geometric and thermodynamic properties in Gauss-Bonnet gravity ⋮ Stability analysis in modified non-local gravity ⋮ Entropy and statefinder diagnosis in chameleon cosmology ⋮ Magnetized anisotropic dark energy cosmological models in scale covariant theory of gravitation ⋮ Stability analysis and observational measurement in 5-D Brans-Dicke cosmology

Cites Work

• Inflationary cosmology with two-component fluid and thermodynamics
• Generalized Brans-Dicke cosmology in the presence of matter and dark energy
• Mach's Principle and a Relativistic Theory of Gravitation
• TIME DEPENDENCE OF BRANS–DICKE PARAMETER ω FOR AN EXPANDING UNIVERSE
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• COSMIC EVOLUTION IN GENERALISED BRANS–DICKE THEORY

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