Model of hybrid star with baryonic and strange quark matter in Tolman-Kuchowicz spacetime
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Publication:6496004
DOI10.1142/S0219887822501043MaRDI QIDQ6496004
Publication date: 2 May 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) Galactic and stellar structure (85A15)
Cites Work
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- A relativistic model for strange quark star
- Sharp bounds on the critical stability radius for relativistic charged spheres
- A new model for strange stars
- Hybrid star model with quark matter and baryonic matter in minimally coupled \(f ( R )\) gravity
- Relativistic strange stars in Tolman-Kuchowicz spacetime
- A comparative analysis of the adiabatic stability of anisotropic spherically symmetric solutions in general relativity
- COMPACT STARS IN HADRON AND QUARK-HADRON MODELS
- A comparison of Hořava–Lifshitz gravity and Einstein gravity through thin-shell wormhole construction
- General Relativistic Fluid Spheres
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- Anisotropic stars in general relativity
- THE STRUCTURE AND FORMATION OF BOSON STARS
- Constant-roll inflation in f(T) teleparallel gravity
- Generalized teleparallel cosmology and initial singularity crossing
- Lattice Universe: examples and problems
- Rotating charged black hole spacetimes in quadratic f(R) gravitational theories
- The contraction of gravitating spheres
- CHARGED AXIALLY SYMMETRIC SOLUTION, ENERGY AND ANGULAR MOMENTUM IN TETRAD THEORY OF GRAVITATION
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Rotating stars in relativity
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