Existence of compact anisotropic stars with Karmarkar-Tolman spacetime

DOI10.1016/J.CJPH.2022.11.010zbMATH Open1545.83139MaRDI QIDQ6545674

M. Sufyan, Daud Ahmad

Publication date: 29 May 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

zbMATH Keywords

\(f(R)\) gravityanisotropic starTolman-Oppenheimer-Volkoff equationcompact starKarmarkar condition

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• \(f(R, T, R_{\mu \nu} T^{\mu \nu})\) gravity phenomenology and \(\lambda\)CDM universe
• Extended gravity description for the GW190814 supermassive neutron star
• Strange stars in \(f(R)\) theories of gravity in the Palatini formalism
• Energy conditions in modified \(f(G)\) gravity
• Dynamics of relativistic fluids with structure scalars and \(\epsilon R^2\) cosmology
• A new type of isotropic cosmological models without singularity
• Static solutions of Einstein's field equations for spheres of fluid.
• Influence of modification of gravity on spherical wormhole models
• Strange stars inf(R,𝒯) gravity
• Modified relativistic dynamics
• Massive spheres in general relativity
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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