Pages that link to "Item:Q5042576"
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The following pages link to Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in f(𝒬) gravity (Q5042576):
Displaying 7 items.
- Relativistic Tolman stellar spheres in \(f(R, \phi)\) theory of gravity (Q6541210) (← links)
- Finch-Skea dark energy stars with vanishing complexity factor (Q6543421) (← links)
- Review on \(f(\mathbb{Q})\) gravity (Q6546551) (← links)
- Anisotropic quark stars in modified \(f(R, T)\) gravity utilizing Tolman V potential (Q6584109) (← links)
- Influence of pressure anisotropy on mass-radius relation and stability of millisecond pulsars in \(f(Q)\) gravity (Q6618122) (← links)
- Most general isotropic charged fluid solution for Buchdahl model in \(\mathscr{F}(\mathcal{Q})\) gravity (Q6618123) (← links)
- Role of decoupling and Rastall parameters on Krori-Barua and Tolman IV models generated by isotropization and complexity factor (Q6646045) (← links)
