RECONSTRUCTING A STRING-INSPIRED NONMINIMALLY COUPLED QUINTOM MODEL

DOI10.1142/S0218271809015096zbMath1181.83253arXiv0811.3343OpenAlexW3102598328MaRDI QIDQ3401080

A. R. Amani, Jafar Sadeghi, Mohammad R. Setare

Publication date: 28 January 2010

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

Full work available at URL: https://arxiv.org/abs/0811.3343

zbMATH Keywords

dark energynonminimal couplingquintom modeltachyonic Lagrangian

Mathematics Subject Classification ID

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

Related Items (6)

Bouncing cosmological models in a functional form of \(F(R)\) gravity ⋮ Thermodynamics of the viscous f(T,B) gravity in the new agegraphic dark energy model ⋮ THERMODYNAMICS OF VISCOUS DARK ENERGY IN AN RSII BRANEWORLD ⋮ The effect of backreaction of non-minimally coupled massless quintom fields in FLRW universe ⋮ Interaction between tachyon and hessence (or hantom) dark energies ⋮ Generalised teleparallel quintom dark energy non-minimally coupled with the scalar torsion and a boundary term

Cites Work

• Generalized second law of thermodynamics in quintom dominated universe
• Cosmic duality in quintom universe
• Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
• Quantum de Sitter cosmology and phantom matter
• Cosmological evolution of the rolling tachyon
• Cosmological constant -- the weight of the vacuum
• The cosmological constant and dark energy
• Dark energy model with spinor matter and its quintom scenario
• Lectures on string/brane cosmology
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The cosmological constant problem
• Assisted inflation via tachyon condensation

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