Anisotropic strange stars in extended \(f(T, B, \mathcal{T})\) gravity with electromagnetic field
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Publication:6549035
DOI10.1016/j.cjph.2023.12.018zbMath1540.83087MaRDI QIDQ6549035
Ujjal Debnath, Krishna pada Das
Publication date: 3 June 2024
Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)
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
- A special exact spherically symmetric solution in f(T) gravity theories
- Teleparallel gravity. An introduction
- Sharp bounds on the critical stability radius for relativistic charged spheres
- Cracking of homogeneous self-gravitating compact objects induced by fluctuations of local anisotropy
- Anisotropic stars. II: Stability
- Over invarianten van bilineaire vormen.
- Een en ander over de energie van het zwaartekrachtsveld volgens de theorie van \textit{Einstein}. (Über die Energie des Schwerefeldes in \textit{Einstein}s Theorie.
- Energy conditions in \(F(T,\varTheta)\) gravity and compatibility with a stable de Sitter solution
- New classes of modified teleparallel gravity models
- Compact anisotropic spheres with prescribed energy density
- Anisotropic relativistic stellar models
- New general relativity
- Cosmological reconstruction of f(T, 𝒯) gravity
- Existence of relativistic stars in f ( T ) gravity
- General Relativistic Fluid Spheres
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- A singularity-free solution for a charged fluid sphere in general relativity
- The amplification of cosmological magnetic fields in extended f(T,B) teleparallel gravity
- Cosmological viable models in f ( T , B ) theory as solutions to the H 0 tension
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- The contraction of gravitating spheres
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
- General solution for a class of static charged spheres
- No further gravitational wave modes in \(F(T)\) gravity
- Dark Energy Star: Physical Constraints on the Bounds
- Preface
- Study of anisotropic strange stars in Krori Barua metric under \(f(T, \mathcal{T})\) gravity
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