Stability of quintom model of dark energy in \((\omega, \omega^{\prime})\) phase plane

DOI10.1007/s10773-011-0808-9zbMath1235.83092OpenAlexW1986875879MaRDI QIDQ763427

A. R. Amani

Publication date: 9 March 2012

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

Full work available at URL: https://doi.org/10.1007/s10773-011-0808-9

zbMATH Keywords

dark energyquintom modelEinstein's equationequation of state parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)

Related Items (5)

Quintom potentials from quantum cosmology using the FRW cosmological model ⋮ Bouncing cosmological models in a functional form of \(F(R)\) gravity ⋮ Anisotropic strange stars with off-diagonal tetrad in f(T,𝒯 ) gravity ⋮ Thermodynamics of the viscous f(T,B) gravity in the new agegraphic dark energy model ⋮ COSMOLOGICAL MODEL OF INTERACTING TACHYON FIELD

Cites Work

• First-order formalism and dark energy
• Quintom cosmologies with arbitrary potentials
• Shape invariance for the bent brane with two scalar fields
• de Sitter brane universe induced by phantom and quantum effects
• Quantum de Sitter cosmology and phantom matter
• Asymptotic behavior of \(\omega\) in general quintom model
• Coupled quintessence and phantom based on a dilaton
• Quintessence with O ( N ) symmetry
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The cosmological constant problem
• Hessence: a new view of quintom dark energy
• Phantom cosmology with general potentials

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