Stability of accelerating cosmology in two scalar-tensor theory: little rip \textit{versus} de Sitter

DOI10.3390/e14081578zbMath1297.83051arXiv1111.5389OpenAlexW2034571441MaRDI QIDQ406149

Sergei D. Odintsov, Shin'ichi Nojiri, Yusaku Ito

Publication date: 8 September 2014

Published in: Entropy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1111.5389

zbMATH Keywords

scalar tensor theorydark energyde Sitter cosmologylittle ripscalar phantom

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (5)

Singular deformations of nearly R ² inflation potentials ⋮ Finite-time cosmological singularities and the possible fate of the universe ⋮ Scalar Field Evolution at Background and Perturbation Levels for a Broad Class of Potentials ⋮ Loop quantum cosmology scalar field models ⋮ Unification of inflation and dark energyà laquintessential inflation

Cites Work

• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Dark Energy
• DYNAMICS OF DARK ENERGY
• More general sudden singularities
• Sudden future singularities
• BIG RIP AND LITTLE RIP SOLUTIONS IN SCALAR MODEL WITH KINETIC AND GAUSS–BONNET COUPLINGS
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• CONSTRAINTS ON THE SOUND SPEED OF DYNAMICAL DARK ENERGY

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