THE BIANCHI TYPE V MAGNETIZED STRING DUST COSMOLOGICAL MODEL IN GENERAL RELATIVITY
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Publication:3500331
DOI10.1142/S0218271807011073zbMath1200.83030OpenAlexW2011290471MaRDI QIDQ3500331
Publication date: 3 June 2008
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0218271807011073
Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (8)
Bianchi V cosmology with a specific Hubble parameter ⋮ Bianchi type I magnetized barotropic perfect fluid cosmological model in general relativity ⋮ Bianchi type V barotropic perfect fluid cosmological model in Lyra geometry ⋮ Bianchi type III cosmological models for barotropic perfect fluid distribution with variable \(G\) and \(\Lambda \) ⋮ LRS Bianchi type II massive string cosmological model for stiff fluid distribution with decaying vacuum energy \((\varLambda)\) ⋮ Investigation of the magnetized string distribution in the Marder universe with the cosmological term in f(R,T) theory ⋮ Bianchi type V cosmological models with constant deceleration parameter in general relativity ⋮ Bianchi type V magnetized string dust bulk viscous fluid cosmological model with variable magnetic permeability
Cites Work
- LRS Bianchi type-V universes filled with matter and radiation
- Bianchi type V perfect-fluid space-times
- Bianchi type V models with a matter distribution admitting ansiotropic pressure and heat flow
- Decomposable differential operators in a cosmological context
- Tilting at cosmological singularities
- Spatially homogeneous and inhomogeneous cosmologies with equation of state p=mu
- L. R. S. Bianchi type I string dust magnetized cosmological models
- Some New General Relativistic Dust Metrics Possessing Isometries
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