Invariant Bianchi type I models in f(R,T) gravity

DOI10.1142/S0219887818500263zbMath1387.83144arXiv1707.03273MaRDI QIDQ4602875

Ahmad T. Ali, Anil Kumar Yadav

Publication date: 7 February 2018

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1707.03273

zbMATH Keywords

invariant solutions\(f(R, T)\) gravityBianchi type - I

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15) Symmetry analysis, Lie group and Lie algebra methods applied to problems in fluid mechanics (76M60)

Related Items (3)

Relationship between magnetic field and anisotropy parameter in gravitation theories ⋮ Accelerating model of a flat universe in \(f(R,T)\) gravity ⋮ Bulk viscous Bianchi-I embedded cosmological model in f(R,T) = f1(R) + f2(R)f3(T) gravity

Cites Work

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• Cylindrically symmetric inhomogeneous universes with a cloud of strings
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• Bianchi type-I model with cosmic string in the presence of a magnetic field: spinor description
• Bianchi type-\(V\) cosmology in \(f(R,T)\) gravity with \(\varLambda (T)\)
• RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES

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