Non-existence of Bianchi type-III bulk viscous string cosmological model in \(f(R,T)\) gravity
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Publication:2443647
DOI10.1007/s10509-013-1459-5zbMath1284.83184OpenAlexW2017783972MaRDI QIDQ2443647
Publication date: 8 April 2014
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-013-1459-5
Relativistic cosmology (83F05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (11)
Bianchi type-V bulk viscous cosmic string in \(f(R, T)\) gravity with time varying deceleration parameter ⋮ Bianchi type-III magnetized string cosmological models for perfect fluid distribution in \(f(R,T)\) gravity ⋮ Stability analysis of stellar radiating filaments ⋮ Energy constraints for static wormholes in f(ℛ,𝒯 ) gravity ⋮ A note on proper conformal vector fields of Bianchi type-I perfect fluid space-times in f(R,T) gravity ⋮ Cosmology in modified f(R,T)-gravity theory in a variant Λ(T) scenario-revisited ⋮ Anisotropic bulk viscous string cosmological model in a scalar-tensor theory of gravitation ⋮ Viscous generalized Chaplygin gas interacting with f(R,T) gravity ⋮ Conformally symmetric traversable wormholes in \(f(R,T)\) gravity ⋮ Axially and reflection symmetric systems and structure scalars in \(f(R,T)\) gravity ⋮ Binary mixture of perfect fluid and dark energy in modified theory of gravity
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