Interacting cosmological viscous fluid with Little Rip and Pseudo Rip solutions in f(R) gravity

DOI10.1142/S0219887818500287zbMath1387.83004OpenAlexW2765820707MaRDI QIDQ4602880

R. D. Boko, M. J. S. Houndjo, Joël Tossa

Publication date: 7 February 2018

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0219887818500287

zbMATH Keywords

bulk viscosityquintessencephantomdark energyredshiftLittle RipPseudo Rip

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Observational and experimental questions in relativity and gravitational theory (83B05) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (1)

Transit cosmological models in modified f(Q,T) gravity

Cites Work

• Dark energy model in anisotropic Bianchi type-III space-time with variable eos parameter
• Bouncing cosmology in modified Gauss-Bonnet gravity
• Casimir effects near the big rip singularity in viscous cosmology
• Le Châtelier-Braun principle in cosmological physics
• Modified \(f(R)\) gravity from scalar-tensor theory and inhomogeneous EoS dark energy
• Generalized Chaplygin gas model: dark energy -- dark matter unification and CMBR con\-straints
• Cosmological constant -- the weight of the vacuum
• Dissipative or conservative cosmology with dark energy?
• Dark energy and viscous cosmology
• Viscous brane cosmology with a brane-bulk energy interchange term
• The cosmological constant and dark energy
• DYNAMICS OF DARK ENERGY
• Bounce universe induced by an inhomogeneous dark fluid coupled with dark matter
• The cosmological constant problem
• The cosmological constant

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