Cosmic acceleration from interaction of ordinary fluids

DOI10.1007/s10714-007-0565-5zbMath1147.83020arXiv0711.3602OpenAlexW2008567629MaRDI QIDQ944942

Bernardo M. O. Fraga, Nelson Pinto-Neto

Publication date: 10 September 2008

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0711.3602

zbMATH Keywords

Cosmic accelerationBouncing universeInteracting fluids

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (4)

Modeling the quantum evolution of the universe through classical matter ⋮ Interacting new generalized Chaplygin gas ⋮ BOUNCE AND WORMHOLES ⋮ Velocity and heat flow in a composite two fluid system

Cites Work

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• Scalar perturbations in regular two-component bouncing cosmologies
• Interacting fluids generating identical, dual and phantom cosmologies
• Anisotropic solutions of the Einstein-Boltzmann equations. I: General formalism
• Statefinder parameters for interacting dark energy
• Relativistic transport theory
• A Suggested Interpretation of the Quantum Theory in Terms of "Hidden" Variables. I
• Interacting quintessence

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