Non-vacuum static cylindrically symmetric solution and energy distribution in \(f(R)\) gravity
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Publication:2348828
DOI10.1007/s10509-012-1150-2zbMath1314.83043OpenAlexW1982475637MaRDI QIDQ2348828
Publication date: 16 June 2015
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-012-1150-2
Relativistic cosmology (83F05) Supergravity (83E50) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (7)
Bianchi type-V domain walls and quark matter cosmological model with cosmological constant \(\Lambda\) in \(f\left(R, T\right)\) gravity ⋮ Gravitational dust collapse in \(f(R)\) gravity ⋮ Classification of static cylindrically symmetric spacetimes in \(f(R)\) theory of gravity by conformal motions with perfect fluid matter ⋮ Some Bianchi type-V accelerating cosmological models in f(R,T) = f1(R) + f2(T) formalism ⋮ Cylindrically symmetric unimodular f(R) black holes ⋮ Non-minimal matter-geometry coupling in the Bianchi-V spacetime within the formalism of f(R, T) = f1(R) + f2(R)f3(T) cosmology ⋮ Bianchi type-\(V\) cosmology in \(f(R,T)\) gravity with \(\varLambda (T)\)
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