Anisotropic stars of class one space-time in \(f(R, \mathcal{T})\) gravity under the simplest linear functional of the matter-geometry coupling
DOI10.1016/J.CJPH.2021.10.040zbMATH Open1539.83073MaRDI QIDQ6542173
Abdelghani Errehymy, Youssef Khedif, G. Mustafa, M. Daoud
Publication date: 21 May 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?)
- An alternative \(f(R,T)\) gravity theory and the dark energy problem
- A relativistic model for strange quark star
- Dynamical instability and the expansion-free condition
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Insufficiency of Karmarkar's condition
- Model astrophysical configurations with the equation of state of Chaplygin gas
- Quark stars in the Einstein-Gauss-Bonnet theory: a new branch of stellar configurations
- Anisotropic quark stars in Einstein-Gauss-Bonnet theory
- General Relativistic Fluid Spheres
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- The contraction of gravitating spheres
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
Related Items (4)
This page was built for publication: Anisotropic stars of class one space-time in \(f(R, \mathcal{T})\) gravity under the simplest linear functional of the matter-geometry coupling
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6542173)