Estimating the role of bag constant and modified theory on anisotropic stellar models
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Publication:6549015
DOI10.1016/J.CJPH.2024.01.012zbMATH Open1545.83054MaRDI QIDQ6549015
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
- Title not available (Why is that?)
- A relativistic model for strange quark star
- \(f(R, T, R_{\mu \nu} T^{\mu \nu})\) gravity phenomenology and \(\lambda\)CDM universe
- Finch-Skea star in \((2+1)\) dimensions
- Evolution of the charged dynamical radiating spherical structures
- Charged anisotropic Finch-Skea-Bardeen spheres
- General Relativistic Fluid Spheres
- CHARGED ANALOGUE OF FINCH–SKEA STARS
- ISOTROPIC CASES OF STATIC CHARGED FLUID SPHERES IN GENERAL RELATIVITY
- Measure of complexity for dynamical self-gravitating structures
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- A charged anisotropic well-behaved Adler–Finch–Skea solution satisfying Karmarkar condition
- Effect of extended gravitational decoupling on isotropization and complexity in f(R,T) theory
- Study of Decoupled Cosmological Solutions in f(R,T)$f(\mathbb {R},\mathbb {T})$ Theory
- Study of Charged Compact Stars in Non‐minimally Coupled Gravity
- Compact objects admitting Finch-Skea symmetry in \(f(\mathcal{R},T^2)\) gravity
- Anisotropic complexity-free models in modified \(f(\mathbf{R},\mathbf{T})\) theory
- Effects of \(f(\mathcal{R}, \mathcal{T}, \mathcal{R}_{\gamma\upsilon}\mathcal{T}^{\gamma\upsilon})\) gravity on anisotropic charged compact structures
- Model of hybrid star with baryonic and strange quark matter in Tolman-Kuchowicz spacetime
Related Items (2)
Extending anisotropic interiors admitting vanishing complexity in charged \(f(\mathbf{R}, \mathbf{T})\) theory ⋮ Role of decoupling and Rastall parameters on Krori-Barua and Tolman IV models generated by isotropization and complexity factor
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