Inflation and bounce from classical and loop quantum cosmology imperfect fluids

DOI10.1142/S0218271817501103zbMath1372.83063arXiv1703.09009MaRDI QIDQ5369094

V. K. Oikonomou

Publication date: 13 October 2017

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

Full work available at URL: https://arxiv.org/abs/1703.09009

zbMATH Keywords

inflationmodified gravityfluid cosmology

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (5)

Finite-time cosmological singularities and the possible fate of the universe ⋮ Loop quantum cosmology-corrected Gauss–Bonnet singular cosmology ⋮ Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state ⋮ Loop quantum cosmology scalar field models ⋮ An extended theory of gravity in a modified Riemann’s geometry

Cites Work

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• Beyond Einstein gravity. A survey of gravitational theories for cosmology and astrophysics.
• A new type of isotropic cosmological models without singularity
• Equation of state for the universe from similarity symmetries
• Loop quantum cosmology: a status report
• F(R)-gravity and inflation
• A nonsingular universe
• Loop quantum gravity effects on inflation and the CMB
• Physical Foundations of Cosmology
• Accelerating cosmology in modified gravity: From convenient F(R) or string-inspired theory to bimetric F(R) gravity

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