Anisotropic stellar solutions in torsion-trace gravity under Karmarkar condition

DOI10.1142/S0219887822500670OpenAlexW4214736066MaRDI QIDQ6196422

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Publication date: 14 March 2024

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

Full work available at URL: https://doi.org/10.1142/s0219887822500670

zbMATH Keywords

compact starsKarmarkar condition\(f(T, \mathcal{T})\) gravitytorsion anisotropic fluid

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

• Unnamed Item
• Geodesic deviation equation in \(\Lambda\)CDM \(f(T,\mathcal {T})\) gravity
• The Hamiltonian constraint in the teleparallel equivalent of general relativity
• Effect of \(f(R)\)-gravity models on compact stars
• A new solution of embedding class I representing anisotropic fluid sphere in general relativity
• General Relativistic Fluid Spheres
• Conformally non-flat spacetime representing dense compact objects
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• The contraction of gravitating spheres
• The cosmological constant problem
• On Massive Neutron Cores

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