Anisotropic stellar filaments evolving under expansion-free condition in f(R,T) gravity

DOI10.1142/S0218271818500475zbMath1427.83075OpenAlexW2783537401MaRDI QIDQ5203788

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Publication date: 9 December 2019

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

Full work available at URL: https://doi.org/10.1142/s0218271818500475

zbMATH Keywords

gravitational collapsedynamical equations\(f(R, T)\) gravityinstability rangezero expansion

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)

Related Items (4)

Study of stellar structures in f(ℛ,𝒯μν𝒯μν) theory ⋮ Panorama behaviors of holographic dark energy models in modified gravity ⋮ Dark energy in spherically symmetric universe coupled with Brans-Dicke scalar field ⋮ Dynamics of shearing viscous fluids in f(R,T) gravity

Cites Work

• Dynamical instability and the expansion-free condition
• Newtonian and post Newtonian expansionfree fluid evolution in \(f(R)\) gravity
• Gravitational perfect fluid collapse in \(f(R)\) gravity
• R ⁿ extension of the Starobinsky model in old minimal supergravity
• Radial pulsations and stability of anisotropic stars with a quasi-local equation of state
• Dynamical instability for non-adiabatic spherical collapse
• EXPANSION-FREE CAVITY EVOLUTION: SOME EXACT ANALYTICAL MODELS
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• Unnamed Item

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