Generalized expanding and shearing anisotropic Bianchi type I magnetofluid cosmological model in general relativity
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Publication:1976380
DOI10.1023/A:1001835420565zbMath0965.83042OpenAlexW226139281MaRDI QIDQ1976380
Publication date: 10 May 2000
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1023/a:1001835420565
magnetic fieldgeneral relativityperfect fluid distributionanisotropic Bianchi type I cosmological model
Relativistic cosmology (83F05) Isotropic turbulence; homogeneous turbulence (76F05) Einstein-Maxwell equations (83C22)
Related Items (10)
BIANCHI TYPE I MAGNETOFLUID COSMOLOGICAL MODELS WITH VARIABLE COSMOLOGICAL CONSTANT REVISITED ⋮ Hypersurface-Homogeneous Cosmological Models with Matter and Dark Energy ⋮ Bianchi type I magnetized barotropic perfect fluid cosmological model in general relativity ⋮ Bianchi type I magnetized stiff fluid models with bulk viscosity in Lyra geometry ⋮ Cyclic anisotropic universe in modified gravity with variable deceleration parameter of third degree ⋮ CLASSICAL AND QUANTUM FEATURES OF THE MIXMASTER SINGULARITY ⋮ Hypersurface-homogeneous bulk viscous fluid space-times with time-dependent cosmological term ⋮ BIANCHI TYPE I MAGNETIZED DUST FILLED UNIVERSE IN LYRA GEOMETRY ⋮ Bianchi type I magnetized tilted imperfect barotropic fluid cosmological models in general relativity ⋮ Some homogeneous Bianchi type IX viscous fluid cosmological models with a varying \(\Lambda\)
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