Tilted LRS Bianchi type-I mesonic stiff fluid cosmological model
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Publication:429903
DOI10.1007/s10773-011-0840-9zbMath1242.83135OpenAlexW1982083784MaRDI QIDQ429903
Publication date: 20 June 2012
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-011-0840-9
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (4)
Tilted Bianchi type III wet dark fluid cosmological model in Saez and Ballester theory ⋮ Tilted Bianchi type-I cosmological model in Lyra geometry ⋮ Mesonic cosmological model with two-fluid source in Lyra geometry ⋮ Tilted Bianchi type-III cosmological models in Lyra geometry
Cites Work
- Bulk viscous L.R.S. Bianchi type V tilted stiff fluid cosmological model in general relativity
- Zero-curvature FRW models and Bianchi I space-time as solutions of the same equation
- Bianchi type-I universe in the presence of zero-mass scalar fields
- Some cylindrically-symmetric cosmological models in general relativity representing viscous fluid and perfect fluid with heat conduction
- Topology and cosmology
- Massive scalar field in the Bianchi type I space time
- Tilted Bianchi type I models with heat conduction filled with disordered radiations of perfect fluid in general relativity
- Tilted cosmological models filled with disordered radiation in general relativity
- LRS Bianchi type I perfect fluid solutions generated from known solutions
- Tilted Bianchi type I stiff fluid magnetized cosmological model in general relativity
- Tilted homogeneous cosmological models
- Bianchi type I cosmological model with a viscous fluid
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