Magnetized stiff fluid cylindrically symmetric universe with two degrees of freedom in general relativity
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Publication:1008120
DOI10.1007/S10773-008-9653-XzbMath1161.83321OpenAlexW1984635484MaRDI QIDQ1008120
Raj Bali, Vimal Chand Jain, Mahbub Ali
Publication date: 24 March 2009
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-008-9653-x
Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)
Related Items (5)
Magnetized emergent universe with null radiation flow ⋮ Viscous Bianchi type I universe with stiff matter and decaying vacuum energy density ⋮ LRS Bianchi type II massive string cosmological model for stiff fluid distribution with decaying vacuum energy \((\varLambda)\) ⋮ Unnamed Item ⋮ Some Bianchi type-II cosmological models in Brans-Dicke theory
Cites Work
- Unnamed Item
- A plane-symmetric solution of Einstein's equations with perfect fluid and an equation of state \(p=\gamma \rho\)
- Stiff magnetofluid cosmological model
- Topology and cosmology
- Plane symmetric self-gravitating fluids with pressure equal to energy density
- Magneto-dilatonic Bianchi-I cosmology: isotropization and singularity problems
- Cylindrical Gravitational News
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