Role of decoupling and Rastall parameters on Krori-Barua and Tolman IV models generated by isotropization and complexity factor
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Publication:6646045
DOI10.1088/1361-6382/ad8d9dMaRDI QIDQ6646045
Publication date: 29 November 2024
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Cites Work
- Les équations de la gravitation einsteinienne.
- Rastall gravity is equivalent to Einstein gravity
- Anisotropic charged strange stars in Krori-Barua spacetime under \(f(R,T)\) gravity
- Anisotropic star models in the context of vanishing complexity
- Evolution of the charged dynamical radiating spherical structures
- Black hole solutions surrounded by perfect fluid in Rastall theory
- Generalization of the Einstein Theory
- General Relativistic Fluid Spheres
- The minimal geometric deformation approach extended
- A singularity-free solution for a charged fluid sphere in general relativity
- The commutator algebra of covariant derivative as general framework for extended gravity. The Rastall theory case and the role of the torsion
- Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in f(đŹ) gravity
- Measure of complexity for dynamical self-gravitating structures
- Cosmology from a new nonconservative gravity
- Gaussian black holes in Rastall gravity
- SEARCHING EXACT SOLUTIONS FOR COMPACT STARS IN BRANEWORLD: A CONJECTURE
- Effect of extended gravitational decoupling on isotropization and complexity in f(R,T) theory
- Relativistic KroriâBarua Compact Stars in f(R,T)$f(R,T)$ Gravity
- Study of Charged Compact Stars in Nonâminimally Coupled Gravity
- More on the fact that Rastall = GR
- Models of non-static and inhomogeneous gravitating source in Rastall gravity
- Complexity of a dynamical dissipative cylindrical system in non-minimally coupled theory
- Constructing traversable wormhole solutions in \(f(R, L_m)\) theory
- Charge effect on isotropization and complexity of extended decoupled anisotropic stellar models
- Extending anisotropic interiors admitting vanishing complexity in charged \(f(\mathbf{R}, \mathbf{T})\) theory
- Estimating the role of bag constant and modified theory on anisotropic stellar models
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