A new class of Bianchi cosmological models in Lyra's geometry
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Publication:352654
DOI10.1007/S10773-012-1382-5zbMath1267.83085OpenAlexW2046492052MaRDI QIDQ352654
Publication date: 5 July 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-012-1382-5
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
Related Items (3)
Phase-plane analysis of FRW cosmological model with variable \(\Lambda\) in Lyra geometry ⋮ Bianchi type-III cosmological models with anisotropic dark energy (DE) in lyra geometry ⋮ Interacting Ricci dark energy models with an effective \(\Lambda\)-term in Lyra manifold
Cites Work
- Cosmological models with linearly varying deceleration parameter
- A new class of LRS Bianchi type-I cosmological models in Lyra geometry
- Anisotropic Bianchi type V perfect fluid cosmological models in Lyra's geometry
- Cosmography: Cosmology without the Einstein equations
- Über eine Modifikation der Riemannschen Geometrie
- AN EXACT BIANCHI TYPE-I COSMOLOGICAL MODEL IN LYRA'S MANIFOLD
- Bianchi type-I cosmological models in Lyra’s geometry
- Jerk, snap and the cosmological equation of state
- A new theory of gravitation
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- A Scalar-Tensor Theory of Gravitation in a Modified Riemannian Manifold
- On the proximate order of $f^{(s)}(z)*g^{(s)}(z)$ and $[f(z)*g(z)^{(s)}$]
- Mach’s principle and the creation of matter
- Early cosmological models in Lyra's geometry
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