Bianchi type-III magnetized string cosmological models for perfect fluid distribution in \(f(R,T)\) gravity

DOI10.1007/s10773-014-2371-7zbMath1325.83009OpenAlexW2122917641MaRDI QIDQ890371

N. E. Zubov

Publication date: 10 November 2015

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10773-014-2371-7

zbMATH Keywords

magnetic field\(f(R,T)\) gravitymassive stringBianchi type-III space-time

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (3)

Magnetized emergent universe with null radiation flow ⋮ Modified Chaplygin gas cosmology with observational constraints ⋮ Unnamed Item

Cites Work

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• Cosmological parameters from SDSS and WMAP
• THE MAGNETIZED UNIVERSE
• Cosmic strings and domain walls

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