Universal relations for anisotropic interacting quark stars
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Publication:6623759
DOI10.1088/1475-7516/2024/10/032MaRDI QIDQ6623759
Publication date: 24 October 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Gravitational waves (83C35)
Cites Work
- A relativistic model for strange quark star
- Relativistic model for anisotropic strange stars
- Holographic compact stars meet gravitational wave constraints
- Approximate universal relations for neutron stars and quark stars
- Relativistic Hydrodynamics
- Radial pulsations and stability of anisotropic stars with a quasi-local equation of state
- Slowly rotating anisotropic neutron stars in general relativity and scalar–tensor theory
- ANALYTICAL MODELS FOR QUARK STARS
- Anisotropic stars in general relativity
- Anisotropic quark stars in f(R) = R 1+ϵ gravity
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
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