Interacting quintessence dark energy models in Lyra manifold
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Publication:2337769
DOI10.1155/2014/878092zbMath1425.83090arXiv1404.2141OpenAlexW3106162333WikidataQ59045137 ScholiaQ59045137MaRDI QIDQ2337769
Antonio Pasqua, Hoda Farahani, Ratbay Myrzakulov, Jafar Sadeghi, Martiros Khurshudyan
Publication date: 20 November 2019
Published in: Advances in High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1404.2141
Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05)
Related Items (6)
Exact cosmological models with Yang-Mills fields on Lyra manifold ⋮ Early and late universe holographic cosmology from a new generalized entropy ⋮ Holographic bounce ⋮ A higher dimensional cosmological model for the search of dark energy source ⋮ Could the Lyra manifold be the hidden source of the dark energy? ⋮ Holographic inflation
Cites Work
- A dark energy model characterized by the age of the Universe
- Effect of varying bulk viscosity on generalized Chaplygin gas
- Cosmological constraints on polytropic gas model
- A universe with a generalized ghost dark energy and van der Waals fluid interacting with a fluid
- Toy models of universe with an effective varying \(\Lambda\)-term in Lyra manifold
- Interacting Ricci dark energy models with an effective \(\Lambda\)-term in Lyra manifold
- Holographic dark energy in braneworld models with a Gauss-Bonnet term in the bulk. Interacting behavior and the \(w=-1\) crossing
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Interacting two-component fluid models with varying EoS parameter
- A TRACKER SOLUTION FOR A HOLOGRAPHIC DARK ENERGY MODEL
- PARAMETRIZATIONS OF THE DARK ENERGY DENSITY AND SCALAR POTENTIALS
- THEORETICAL ASPECTS OF QUINTOM MODELS
- Cosmological evolution with interaction between dark energy and dark matter
- QUINTOM COSMOLOGY WITH GENERAL POTENTIALS
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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