Bianchi type III and Kantowski-Sachs cosmological models in Lyra geometry
From MaRDI portal
Publication:1180204
DOI10.1007/BF00644115zbMath0735.76095WikidataQ125862801 ScholiaQ125862801MaRDI QIDQ1180204
Publication date: 27 June 1992
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Related Items (4)
Bianchi type-III cosmological models with time dependent displacement vector for barotropic fluid distribution in Lyra geometry ⋮ Anisotropic Bianchi type V perfect fluid cosmological models in Lyra's geometry ⋮ A new class of LRS Bianchi type-I cosmological models in Lyra geometry ⋮ Bianchi type V and \(VI_ 0\) cosmological models in Lyra geometry
Cites Work
- Bianchi type V and \(VI_ 0\) cosmological models in Lyra geometry
- Solutions to Einstein's field equations with Kantowski-Sachs symmetry and string dust source
- Lorentzian 4 dimensional manifolds with 'local isotropy'
- Über eine Modifikation der Riemannschen Geometrie
- Relativistic Cosmology. I
- On Geodesics of a Modified Riemannian Manifold
- A Scalar-Tensor Theory of Gravitation in a Modified Riemannian Manifold
This page was built for publication: Bianchi type III and Kantowski-Sachs cosmological models in Lyra geometry
