Dark energy model with variable \(q\) and \(\omega\) in LRS Bianchi-II space-time
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Publication:2443610
DOI10.1007/s10509-012-1070-1zbMath1284.83206arXiv1110.4887OpenAlexW2124939784MaRDI QIDQ2443610
Publication date: 8 April 2014
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1110.4887
Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (8)
Hypersurface-Homogeneous Cosmological Models with Matter and Dark Energy ⋮ Holographic dark energy model with quintessence in Bianchi type-I space-time ⋮ Anisotropic viscous fluid cosmological models from deceleration to acceleration in string cosmology ⋮ Holographic dark energy (DE) cosmological models with quintessence in Bianchi type-V space time ⋮ Nonlinear spinor fields in Bianchi type-I spacetime reexamined ⋮ Magnetised strings in \(\lambda\)-dominated anisotropic universe ⋮ Whether dark energy can contribute to the treatment and healing of diseases ⋮ \(\Lambda\) CDM-type cosmological model and observational constraints
Cites Work
- LRS Bianchi-I anisotropic cosmological model with dominance of dark energy
- LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
- Bianchi type III models with anisotropic dark energy
- Dark energy models with variable equation of state parameter
- Bianchi type III anisotropic dark energy models with constant deceleration parameter
- The Bianchi models: then and now
- SOME BIANCHI TYPE-V MODELS OF ACCELERATING UNIVERSE WITH DARK ENERGY
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
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