PARAMETRIZATION OF TACHYON FIELD

DOI10.1142/S0217732307021809zbMath1117.85015arXivgr-qc/0703112MaRDI QIDQ5292315

Wei Wang, Ying Shao, Yuan Xing Gui

Publication date: 20 June 2007

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0703112

zbMATH Keywords

parametrizationreconstructionequation of statetachyon field

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (9)

Polytropic gas scalar field models of dark energy ⋮ Spinor model of a perfect fluid and their applications in Bianchi type-I and FRW models ⋮ Scalar field in cosmology: potential for isotropization and inflation ⋮ STATEFINDER DIAGNOSTIC FOR COUPLED TACHYON DARK ENERGY MODEL ⋮ Interacting Ricci dark energy with logarithmic correction ⋮ Behavior of holographic Ricci dark energy in scalar Gauss-Bonnet gravity for different choices of the scale factor ⋮ INTERACTING HOLOGRAPHIC TACHYON MODEL OF DARK ENERGY ⋮ Cosmological implications of interacting polytropic gas dark energy model in non-flat universe ⋮ RECONSTRUCTING THE POTENTIALS FOR THE QUINTESSENCE AND TACHYON DARK ENERGY, FROM THE HOLOGRAPHIC PRINCIPLE

Cites Work

• Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
• Cosmological evolution of the rolling tachyon
• Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
• Cosmological dynamics of the tachyon with an inverse power-law potential
• \(k\)-inflation
• Tachyon couplings on non-BPS D-branes and Dirac-Born-Infeld action
• An alternative to quintessence

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