Properties of interacting quark star in light of Rastall gravity
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Publication:6660884
DOI10.1088/1361-6382/ad9c0fMaRDI QIDQ6660884
Archana Dixit, İzzet Sakallı, Anirudh Pradhan, Ayan Banerjee
Publication date: 10 January 2025
Published in: Classical and Quantum Gravity (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
- The stability of relativistic stars and the role of the adiabatic index
- Holographic compact stars meet gravitational wave constraints
- Modified theories of gravity: why, how and what?
- Lagrangian formalism for Rastall theory of gravity and Gödel-type universe
- Generalization of the Einstein Theory
- The stability of relativistic gas spheres⋆
- Shadow cast of noncommutative black holes in Rastall gravity
- Emergent cosmic space in Rastall theory
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
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