Bianchi type I magnetized stiff fluid models with bulk viscosity in Lyra geometry
DOI10.1007/s40010-013-0087-3zbMath1329.83146OpenAlexW2035194771MaRDI QIDQ893459
Publication date: 19 November 2015
Published in: Proceedings of the National Academy of Sciences, India. Section A. Physical Sciences (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s40010-013-0087-3
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Electromagnetic theory (general) (78A25) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Cites Work
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- Bulk viscous Bianchi type I cosmological models with time-dependent cosmological term \(\Lambda \)
- Magnetized cosmological model
- Plane symmetric domain wall in Lyra geometry
- Generalized expanding and shearing anisotropic Bianchi type I magnetofluid cosmological model in general relativity
- Über eine Modifikation der Riemannschen Geometrie
- BIANCHI TYPE I MAGNETIZED DUST FILLED UNIVERSE IN LYRA GEOMETRY
- Magneto-dilatonic Bianchi-I cosmology: isotropization and singularity problems
- HIGHER DIMENSIONAL COSMOLOGICAL MODEL IN LYRA GEOMETRY
- Bianchi type-I cosmological model for perfect fluid distribution in Lyra geometry
- Cylindrically symmetric viscous fluid universe in Lyra geometry
- Bianchi type-I cosmological models in Lyra’s geometry
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