Tachyon field as a dark energy in Bianchi type-V spacetime
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Publication:5174274
DOI10.1142/S021773231550008XzbMath1305.83064arXiv1404.3860OpenAlexW2066060881MaRDI QIDQ5174274
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Publication date: 17 February 2015
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1404.3860
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Related Items (3)
Interacting holographic dark energy in Bianchi type-V and IX universes with variable deceleration parameter ⋮ Scalar field and time varying cosmological constant in \(f(R, T)\) gravity for Bianchi type-I universe ⋮ Thermodynamics of the viscous f(T,B) gravity in the new agegraphic dark energy model
Cites Work
- Effect of varying bulk viscosity on generalized Chaplygin gas
- Generalized second law of thermodynamics in quintom dominated universe
- Holographic Chaplygin gas model
- Cosmological evolution of the rolling tachyon
- Modified Chaplygin gas cosmology
- Interacting entropy-corrected holographic dark energy and IR cut-off length
- Time-dependent density of modified cosmic Chaplygin gas with variable cosmological constant in non-flat universe
- COSMOLOGICAL MODELS WITH A VARYING Λ-TERM IN LYRA'S GEOMETRY
- Interacting two-component fluid models with varying EoS parameter
- SOME BIANCHI TYPE-V MODELS OF ACCELERATING UNIVERSE WITH DARK ENERGY
- DYNAMICS OF DARK ENERGY
- PARAMETRIZATIONS OF THE DARK ENERGY DENSITY AND SCALAR POTENTIALS
- Role of modified Chaplygin gas in accelerated universe
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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