Relativistic model for anisotropic spheres in \(f(R,T)\) gravity via Karmarkar condition

DOI10.1016/J.AOP.2021.168622zbMath1482.85008OpenAlexW3202143637MaRDI QIDQ2058642

Yanyan Li

Publication date: 9 December 2021

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.aop.2021.168622

zbMATH Keywords

\(f(R,T)\) gravity theorycompact starsKarmarkar condition

Mathematics Subject Classification ID

Gravitational energy and conservation laws; groups of motions (83C40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)

Cites Work

• Collapsing shear-free perfect fluid spheres with heat flow
• Anisotropic fluid spheres in the framework of \(f(R,T)\) gravity theory
• Anisotropic stars for spherically symmetric spacetimes satisfying the Karmarkar condition
• General Relativistic Fluid Spheres
• Superfluidity and the moments of inertia of nuclei
• Exact model for a relativistic star
• Bounds on the basic physical parameters for anisotropic compact general relativistic objects
• Exact Solutions of Einstein's Field Equations
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• The contraction of gravitating spheres
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• On Massive Neutron Cores

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