Tolman IV fluid sphere in \(f(R, T)\) gravity

DOI10.1016/j.cjph.2021.11.013zbMath1539.8306MaRDI QIDQ6542241

P. Bhar, Unnamed Author, M. Zubair

Publication date: 21 May 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

zbMATH Keywords

adiabatic indexcausality conditioncompact star\(f(R, T)\) gravity

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (5)

Charged anisotropic fluid sphere in \(f(\mathcal{R}, T)\) gravity ⋮ Celestial attributes of hybrid star in \(5\mathcal{D}\) Einstein-Gauss-Bonnet gravity ⋮ Stellar structure modeling in Ricci-inverse gravity with Tolman-Kuchowicz spacetime ⋮ Tolman IV perfect fluid sphere in Rastall gravity ⋮ Investigating the equation-of-state, stability and mass-radius relationship of anisotropic and massive neutron stars embedded in \(f(R, T)\) modified gravity

Cites Work

• Some anisotropic cosmological models in a modified theory of gravitation
• Charge analogue of Tolman IV solution for anisotropic fluid
• A new type of isotropic cosmological models without singularity
• General Relativistic Fluid Spheres
• Bounds on the basic physical parameters for anisotropic compact general relativistic objects
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• The Highly Collapsed Configurations of a Stellar Mass
• The Highly Collapsed Configurations of a Stellar Mass. (Second Paper.)
• RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
• Dynamics of shearing viscous fluids in f(R,T) gravity
• Modified relativistic dynamics
• Cosmological consequences and statefinder diagnosis of a noninteracting generalized Chaplygin gas in f(R,T) gravity
• A note on covariant conservation of energy–momentum in modified gravities
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• Finch–Skea star model in f(R,T) theory of gravity
• Modelling of dark energy stars with Tolman IV gravitational potential

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