Can an interacting varying Chaplygin gas and tachyonic matter accelerate universe?

DOI10.1142/S0219887818501554zbMath1395.83140arXiv1301.4990MaRDI QIDQ4585792

Martiros Khurshudyan

Publication date: 7 September 2018

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

Full work available at URL: https://arxiv.org/abs/1301.4990

zbMATH Keywords

expanding universedark fluid modelfuture singularitie

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (9)

Viscous varying generalized Chaplygin gas with cosmological constant and space curvature ⋮ Time-dependent density of modified cosmic Chaplygin gas with variable cosmological constant in non-flat universe ⋮ Phenomenological fluids from interacting tachyonic scalar fields ⋮ Viscous new varying modified cosmic Chaplygin gas with cosmological constant in non-flat universe ⋮ Interacting modified cosmic Chaplygin gas with variable cosmological constant and viscosity ⋮ Ghost dark energy with sign-changeable interaction term ⋮ Generalized logarithmic equation of state in classical and loop quantum cosmology dark energy-dark matter coupled systems ⋮ Type V singularities with inhomogeneous equations of state ⋮ Holographic Dark Energy with Extended Chaplygin Gas Model

Cites Work

• σCDM coupled to radiation: Dark energy and Universe acceleration

This page was built for publication: Can an interacting varying Chaplygin gas and tachyonic matter accelerate universe?