Magnetized emergent universe with null radiation flow
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Publication:267268
DOI10.1007/s10773-015-2655-6zbMath1337.83110OpenAlexW2048129649MaRDI QIDQ267268
F. Blanchet-Sadri, M. Dambrine
Publication date: 8 April 2016
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-015-2655-6
Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Electromagnetic theory (general) (78A25) Radiative transfer in astronomy and astrophysics (85A25)
Cites Work
- Spatially homogeneous Bianchi type-I universes with variable \(G\) and \(\Lambda \)
- Bianchi type-III magnetized string cosmological models for perfect fluid distribution in \(f(R,T)\) gravity
- Magnetized stiff fluid cylindrically symmetric universe with two degrees of freedom in general relativity
- A rotating mass particle embedded in a Bianchi type IX universe
- Modified Chaplygin gas cosmology with statefinder diagnostic in Lyra geometry
- Some spatially homogeneous string cosmological models
- Bianchi type-III cosmological models in Lyra's geometry in the presence of massive scalar field
- Some cosmological models with heat and null radiation flow
- Emergent universe with exotic matter
- Emergent universe and the phantom tachyon model
- The emergent universe: inflationary cosmology with no singularity
- The emergent universe: an explicit construction
- Isotropic loop quantum cosmology