Bianchi type-I bulk viscous cosmology with Chaplygin gas in Lyra geometry
From MaRDI portal
Publication:6122101
DOI10.1016/j.cjph.2016.10.005OpenAlexW2534712134MaRDI QIDQ6122101
Binaya K. Bishi, P. K. Sahoo, G. P. Singh
Publication date: 28 February 2024
Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/j.cjph.2016.10.005
Cites Work
- A cosmological model of the early universe based on ECG with variable \(\Lambda\)-term in Lyra geometry
- New class of magnetized inhomogeneous Bianchi type-I cosmological model with variable magnetic permeability in Lyra geometry
- A new class of LRS Bianchi type-I cosmological models in Lyra geometry
- Holographic Chaplygin gas model
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Density perturbations in a universe dominated by the Chaplygin gas
- Modified Chaplygin gas cosmology with statefinder diagnostic in Lyra geometry
- Kantowski-Sachs cosmological model in Lyra's geometry
- Anisotropic Bianchi type-III bulk viscous fluid universe in Lyra geometry
- Tilted Bianchi type-III cosmological models in Lyra geometry
- Homothetic motion in a Bianchi type-I model in Lyra geometry
- Über eine Modifikation der Riemannschen Geometrie
- Homothetic vector field in plane symmetric Bianchi type-I cosmological model in Lyra geometry
- Mach's Principle and a Relativistic Theory of Gravitation
- AN EXACT BIANCHI TYPE-I COSMOLOGICAL MODEL IN LYRA'S MANIFOLD
- Mach’s principle and the creation of matter
- An alternative to quintessence