Dynamical stability in scalar-tensor cosmology

DOI10.1007/S10509-011-0920-6zbMath1238.83074arXiv1111.1305OpenAlexW3100862317MaRDI QIDQ422268

Amin Salehi, Ali Shahabi, Hossein Farajollahi

Publication date: 16 May 2012

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1111.1305

zbMATH Keywords

stabilityattractordistance modulusphantom crossingquintomscalar tensor

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (2)

Quintom potentials from quantum cosmology using the FRW cosmological model ⋮ BRANS–DICKE CHAMELEONIC COSMOLOGY AND COSMIC EVOLUTION

Cites Work

• Stability analysis in modified non-local gravity
• Modified gravity with ln \(R\) terms and cosmic acceleration
• The holographic dark energy in non-flat Brans-Dicke cosmology
• TIME DEPENDENCE OF BRANS–DICKE PARAMETER ω FOR AN EXPANDING UNIVERSE
• QUINTOM COSMOLOGY WITH GENERAL POTENTIALS
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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