The mass-radius relation for quark stars in energy-momentum squared gravity
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Publication:2103249
DOI10.1016/j.aop.2022.169149OpenAlexW4307111898MaRDI QIDQ2103249
Indrani Karar, Takol Tangphati, Anirudh Pradhan, Ayan Banerjee
Publication date: 13 December 2022
Published in: Annals of Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2206.10371
Cites Work
- Nonperturbative models of quark stars in \(f(R)\) gravity
- Quark stars in the Einstein-Gauss-Bonnet theory: a new branch of stellar configurations
- Structure of magnetized strange quark star in perturbative QCD
- Anisotropic quark stars in Einstein-Gauss-Bonnet theory
- Anisotropic quark stars in \(R^2\) gravity
- Extended theories of gravity and their cosmological and astrophysical applications
- The stability of relativistic gas spheres⋆
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
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