Energy bounds in \(f(R, T)\) gravity with anisotropic backgrounds
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Publication:6665233
DOI10.1142/S0219887824502396MaRDI QIDQ6665233
Publication date: 17 January 2025
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
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- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- An exponential \(F(R)\) dark energy model
- DARK ENERGY MODELS TOWARD OBSERVATIONAL TESTS AND DATA
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Charged perfect fluid gravitational collapse in f(R, T) gravity
- Relativistic Krori‐Barua Compact Stars in f(R,T)$f(R,T)$ Gravity
- Electromagnetic effects on anisotropic expansion-free fluid content
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- Bouncing cosmology with 4D-EGB gravity
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- Singularity-free anisotropic compact star in \(f(R, \phi)\) gravity via Karmarkar condition
- Noncommutative wormhole solutions in modified \(f(R)\) theory of gravity
- Study of embedded class-i fluid spheres in \(f(R, T)\) gravity with Karmarkar condition
- Relativistic Tolman stellar spheres in \(f(R, \phi)\) theory of gravity
- Bouncing cosmology in Chern-Simons \(f(R)\) gravity
- Stellar structure modeling in Ricci-inverse gravity with Tolman-Kuchowicz spacetime
- Impact of \(f(Q)\) gravity on anisotropic compact star model and stability analysis
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