Analysis of charged compact stars in f(R,T) gravity using Bardeen geometry
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Publication:6188795
DOI10.1142/S0219887823500615MaRDI QIDQ6188795
Munsif Jan, Unnamed Author, Unnamed Author, A. Malik, Muhammad Rizwan Shahzad
Publication date: 11 January 2024
Published in: International Journal of Geometric Methods in Modern Physics (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
- Nonperturbative models of quark stars in \(f(R)\) gravity
- Dark \(f(\mathcal{R},\varphi,\chi)\) universe with Noether symmetry
- GEODESIC STRUCTURE OF TEST PARTICLE IN BARDEEN SPACETIME
- Tolman–Oppenheimer–Volkoff equations in nonlocal f(R) gravity
- PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
- Energy and momentum of a spherically symmetric dilaton frame as regularized by teleparallel gravity
- General Relativistic Fluid Spheres
- Behavior of Anisotropic Compact Stars in f(R, ϕ) Gravity*
- Mimetic compact stars
- Constant-roll inflation in f(T) teleparallel gravity
- Generalized teleparallel cosmology and initial singularity crossing
- Rotating AdS black holes in Maxwell- f ( T ) gravity
- Rotating charged black hole spacetimes in quadratic f(R) gravitational theories
- Analysis of charged compact stars in modified gravity
- Bardeen–de Sitter black holes
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- CHARGED AXIALLY SYMMETRIC SOLUTION, ENERGY AND ANGULAR MOMENTUM IN TETRAD THEORY OF GRAVITATION
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
- The Bardeen model as a nonlinear magnetic monopole
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