Interacting tachyon dark energy in non-flat universe

Abstract

In this paper we study the tachyon cosmology in non-interacting and interacting cases in non-flat FRW universe. Then we reconstruct the potential and the dynamics of the tachyon field which describe tachyon cosmology.

10 pages, 2 figures. Version to appear in PLB (2009)

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Cited by in corpus (50)

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• Two-Fluid Scenario for Dark Energy Models in an FRW Universe-Revisited
• Interacting agegraphic tachyon model of dark energy
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• Statefinder diagnostic and stability of modified gravity consistent with holographic and new agegraphic dark energy
• An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe
• The bouncing cosmology with $F(R)$ gravity and its reconstructing
• Interacting entropy-corrected agegraphic-tachyon dark energy
• Interacting Entropy-Corrected Holographic Dark Energy and IR Cut-Off Length
• Correspondence between DBI-essence and Modified Chaplygin Gas and the Generalized Second Law of Thermodynamics
• Bounce cosmology in $f(\mathcal{R})$ gravity
• Bouncing Universe and Reconstructing Vector Field
• Thermodynamics of the viscous $f(T,B)$ gravity in the new agegraphic dark energy model
• Viscous Generalized Chaplygin Gas Interacting with f(R,T) gravity
• Interaction between viscous varying modified cosmic Chaplygin gas and Tachyonic fluid
• Cosmology of a generalised version of holographic dark energy in presence of bulk viscosity and its inflationary dynamics through slow roll parameters
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• Thermodynamics and stability of $f(T,B)$ gravity with viscous fluid by observational constraints
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Stability and interacting $f(T,\mathcal{T})$ gravity with modified Chaplygin gas
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• Interacting Ricci Dark Energy and its Statefinder Description
• Interacting agegraphic dark energy model in tachyon cosmology coupled to matter
• Improved dynamics and gravitational collapse of tachyon field coupled with a barotropic fluid
• Logarithmic entropy corrected holographic dark energy with $F(R,T)$ gravity
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• A Dark Energy Quintessence Model of the Universe
• Evolution of shifted cosmological parameter and shifted dust matter in a two-phase tachyonic field universe
• Modelling Tachyon Cosmology with Non-Minimal Derivative Coupling to Gravity
• Cosmological Model of Interacting Tachyon Field
• Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory
• Cosmic expansion driven by real scalar field for different forms of potential
• The universe dynamics in the tachyon cosmology with non-minimal coupling to matter
• Bouncing cosmological models in a functional form of F(R) gravity
• Perturbed dark energy: classical scalar field versus tachyon
• Observational constraints and stability in viscous $f(T,\mathcal{T})$ gravity
• Extended Bose-Einstein condensate dark matter in viscous Gauss-Bonnet gravity
• The interaction of extended Bose-Einstein condensate dark matter with viscous $f(T,B)$ gravity
• Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
• Generalized second law of thermodynamics in presence of interacting tachyonic field and scalar(phantom)field
• Evolution of spherical over-densities in tachyon scalar field model
• Interacting Kasner-type cosmologies
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Interacting Viscous Dark Energy in Bianchi Type-III Universe
• Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
• Evolution of spherical overdensities in new agegraphic dark energy model
• Inflation via logarithmic entropy-corrected holographic dark energy model
• Interaction between Tachyon and Hessence (or Hantom) dark energies
• Study of Tachyonic Field and its statefinder diagnostics in Various Scenarios of The Anisotropic Universe