Anisotropic Quark Stars in Modified $f(R,T)$ Gravity utilizing Tolman V potential
Tayyaba Naz, Adnan Malik, Zenab Ramay

TL;DR
This paper explores anisotropic quark star models within modified $f(R,T)$ gravity using Tolman V potential, analyzing their physical properties, stability, and consistency with observational data, thus extending Einstein's gravity in stellar astrophysics.
Contribution
It introduces a novel model of anisotropic quark stars in $f(R,T)$ gravity with Tolman V potential, incorporating the MIT bag model and observational data to validate the physical viability.
Findings
Model satisfies physical and stability conditions.
Bag constant aligns with experimental data.
Energy density and pressures are consistent with observed stars.
Abstract
Alternative gravity theory is currently an incredibly significant technique for addressing some enduring experimental difficulties, such as the universe's dark region. They may also be employed in celestial cosmology, producing results that are a stage beyond those found using Einstein's General Relativity. In this study, we examine the characteristics of anisotropic spherically symmetric stellar structures in the context of modified gravity. In order to explain the distinctive characteristics of compact objects, we investigate how the fluid distribution in the star model is affected by the MIT bag model equation of state. By using Tolman V metric potentials, we establish the field equations, and by employing the experimental data of the three observed stars, we identify the values of unknown parameters. By using a realistic model, we investigate the effect of the…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Cosmology and Gravitation Theories
