Domain wall cosmological models with deceleration parameter in modified theory of gravitation

DOI10.1016/J.CJPH.2016.05.005OpenAlexW2465369976MaRDI QIDQ6121138

S. D. Katore, S. P. Hatkar, R. J. Baxi

Publication date: 26 February 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.cjph.2016.05.005

zbMATH Keywords

domain wallsFriedmann-Robertson-Walkeraxially symmetric\(f(R, T)\) gravity

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (1)

Transit cosmological models with domain walls in \(f(R,T)\) gravity

Cites Work

• LRS Bianchi type-II universe with cosmic strings and bulk viscosity in a modified theory of gravity
• Cosmological models with linearly varying deceleration parameter
• Uniform anisotropic cosmological model with string source
• Domain walls strange quark matter in Einstein-Rosen space-time with cosmological constant and heat flow
• Domain walls in \(f(R,T)\) theory of gravitation
• Five dimensional domain walls in a scalar-tensor theory of gravitation
• Cylindrically symmetric and inhomogeneous cosmological models with viscous fluid, heat flux and electromagnetic field
• Cosmic strings and domain walls in a scale-covariant theory of gravitation
• Axially symmetric non-static domain walls in scalar-tensor theories of gravitation
• Bianchi type III and Kantowski–Sachs domain wall cosmological models in the f(R, T) theory of gravitation

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