Newtonian and post Newtonian expansionfree fluid evolution in \(f(R)\) gravity
DOI10.1007/S10509-011-0863-YzbMath1238.83055arXiv1201.2093OpenAlexW3098967938MaRDI QIDQ422251
Publication date: 16 May 2012
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1201.2093
Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)
Related Items (3)
Cites Work
- Non-vacuum solutions of Bianchi type \(VI _{0}\) universe in \(f(R)\) gravity
- \(d\)-dimensional non-asymptotically flat thin-shell wormholes in Einstein-Yang-Mills-dilaton gravity
- \(f(R)\) black holes
- Can modified gravity explain accelerated cosmic expansion?
- \(1/R\) gravity and scalar-tensor gravity
- Gravitational perfect fluid collapse in \(f(R)\) gravity
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- EFFECTS OF f(R) DARK ENERGY ON DISSIPATIVE ANISOTROPIC COLLAPSING FLUID
- Cavity evolution in relativistic self-gravitating fluids
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
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