Anisotropic stellar model in \(F(T, \mathcal{T})\) gravity under the Karmarkar condition

DOI10.1142/S0219887822500566MaRDI QIDQ6492651

E. Güdekli, Unnamed Author, Iftikhar Ahmed, M. Junaid Kamran

Publication date: 25 April 2024

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

zbMATH Keywords

anisotropic starsTolman-Oppenheimer-Volkov equationKarmarkar condition\(F(T, \mathcal{T})\) gravity

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

• The Hamiltonian constraint in the teleparallel equivalent of general relativity
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• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
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• Classes of exact Einstein-Maxwell solutions
• New general relativity
• Cosmological reconstruction of f(T, 𝒯) gravity
• Reconstruction, thermodynamics and stability of the ΛCDM model in $f(T,{ \mathcal T })$ gravity
• General Relativistic Fluid Spheres
• Mach's Principle and a Relativistic Theory of Gravitation
• TORSION GRAVITY: A REAPPRAISAL
• Solar system tests in modified teleparallel gravity
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• On Massive Neutron Cores
• On Continued Gravitational Contraction

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